diff --git a/.rubocop_todo.yml b/.rubocop_todo.yml index 984ae86..28ef19c 100644 --- a/.rubocop_todo.yml +++ b/.rubocop_todo.yml @@ -1,6 +1,6 @@ # This configuration was generated by # `rubocop --auto-gen-config` -# on 2026-05-05 13:10:07 UTC using RuboCop version 1.86.1. +# on 2026-05-05 23:57:36 UTC using RuboCop version 1.86.1. # The point is for the user to remove these configuration records # one by one as the offenses are removed from the code base. # Note that changes in the inspected code, or installation of new diff --git a/CHANGELOG.md b/CHANGELOG.md index 79ba511..d023553 100644 --- a/CHANGELOG.md +++ b/CHANGELOG.md @@ -1,5 +1,37 @@ ## [Unreleased] +### Added + +- `Tbx::DataElement` shared concern — DRY module injecting common data-category + attributes (id, lang, target, datatype, type, content) via `included` hook +- `Tbx::DataElement::InlineContent` sub-concern for elements with `entity.noteText` + content model (hi, ec, foreign, ph, sc inline children) +- `Tbx::Modules::Min` — Min module TYPES/VALUES constants (Min.tbxmd) +- `Tbx::Modules::Basic` — Basic module TYPES/VALUES constants (Basic.tbxmd) +- `Tbx::Modules::Linguist` — Linguist module TYPES/VALUES constants (Linguist.tbxmd) +- `Tbx::Modules::CoreTypes` — Core RNG hi type constants +- TYPES constants on all data-category elements (Admin, AdminNote, Descrip, + TermNote, Ref, Xref, Transac, TransacNote, Hi), composed from module hashes +- VALUES constants on TermNote (picklist enums) and Transac (transaction types) +- `Tbx::TermComp` — term component element `` (TermComp module) +- `Tbx::TermCompGrp` — term component group `` (TermComp module) +- `Tbx::TermCompSec` — term component section `` (TermComp module) + with TYPES for 5 decomposition methods +- Comprehensive YARD RubyDoc on all element classes tracing schema/module sources +- 119 new specs (165 total) covering TYPES/VALUES, DataElement concern, and + XML round-trips for all data-category elements and TermComp elements + +### Changed + +- Data-category elements (Admin, Descrip, TermNote, AdminNote, DescripNote, + TransacNote, Transac, Ref) now use `include Tbx::DataElement` instead of + explicit attribute declarations +- `Tbx::TermNote::TYPES` now composes from Min + Basic + Linguist (9 types) +- `Tbx::Sc` aligned with core RNG: removed type, subtype, target attributes + (only id and isolated per RNG) +- Reference documentation downloaded from 12 LTAC-Global repositories into + `reference-docs/schemas/` with acknowledgements + ## [0.1.1] - 2026-05-05 - Simplify `Tbx::Namespaces::TbxNamespace` to `Tbx::Namespace` diff --git a/CLAUDE.md b/CLAUDE.md index f80cf68..a0f75e4 100644 --- a/CLAUDE.md +++ b/CLAUDE.md @@ -45,6 +45,9 @@ Tbx ├── LangSec # ├── TermSec # ├── Term # +├── TermComp # (TermComp module) +├── TermCompGrp # (TermComp module) +├── TermCompSec # (TermComp module) ├── TermNote # ├── TermNoteGrp # ├── Descrip # @@ -72,7 +75,13 @@ Tbx ├── Sc # ├── Ph # ├── Title # -└── Namespace # XML namespace definition (urn:iso:std:iso:30042:ed-2) +├── DataElement # Shared concern for data-category elements +├── Namespace # XML namespace (urn:iso:std:iso:30042:ed-2) +└── Modules + ├── Min # Min module TYPES/VALUES + ├── Basic # Basic module TYPES/VALUES + ├── Linguist # Linguist module TYPES/VALUES + └── CoreTypes # Core RNG hi types ``` ### Key Implementation Patterns @@ -105,6 +114,17 @@ end **Autoload Pattern**: Elements are autoloaded via `lib/tbx.rb`. When adding new elements, add autoloads in alphabetical order. +**DataElement Concern** (`lib/tbx/data_element.rb`): +- `Tbx::DataElement` — injects shared attributes (id, lang, target, datatype, type, content) via `self.included(base)` hook +- `Tbx::DataElement::InlineContent` — adds inline child attributes (hi, ec, foreign, ph, sc) for elements with `entity.noteText` content +- XML mappings remain explicit per class (lutaml-model's `xml do` uses `instance_eval` on a separate context) +- Included by: Admin, Descrip, TermNote (with InlineContent); AdminNote, DescripNote, TransacNote, Transac, Ref (without) + +**Module TYPES/VALUES** (`lib/tbx/modules/`): +- Each module defines `*_TYPES` and `*_VALUES` hashes keyed by Ruby symbol, valued by TBX string +- Element classes compose TYPES via `merge` from all applicable modules (e.g., `TermNote::TYPES` merges Min + Basic + Linguist) +- Source: Min.tbxmd, Basic.tbxmd, Linguist.tbxmd, TBXcoreStructV03.rng + ### XML Namespace The TBX namespace is `urn:iso:std:iso:30042:ed-2` defined in `Tbx::Namespace`. diff --git a/README.adoc b/README.adoc index a92c455..e3458e9 100644 --- a/README.adoc +++ b/README.adoc @@ -89,44 +89,386 @@ tbx.to_xml tbx.to_xml(pretty: true, declaration: true, encoding: "utf-8") ---- -=== Supported TBX elements +=== Using TYPES and VALUES constants -==== Root and structure +Each data-category element class exposes `TYPES` (permitted `@type` values) +and `VALUES` (permitted picklist values) constants composed from the +TBX module definitions: -`Document` (`<tbx>`), `TbxHeader`, `TextElement`, `Body`, `Back` +[source,ruby] +---- +# Permitted termNote types across all modules +Tbx::TermNote::TYPES +# => { administrative_status: "administrativeStatus", part_of_speech: "partOfSpeech", +# geographical_usage: "geographicalUsage", grammatical_gender: "grammaticalGender", +# term_location: "termLocation", term_type: "termType", +# grammatical_number: "grammaticalNumber", register: "register", +# transfer_comment: "transferComment" } + +# Picklist values for a specific type +Tbx::TermNote::VALUES[:grammatical_gender] +# => { masculine: "masculine", feminine: "feminine", neuter: "neuter", other: "other" } + +# Admin types from all modules +Tbx::Admin::TYPES +# => { customer_subset: "customerSubset", project_subset: "projectSubset", +# source: "source", reading: "reading" } + +# Descrip types +Tbx::Descrip::TYPES +# => { subject_field: "subjectField", context: "context", definition: "definition" } + +# Hi types from core RNG +Tbx::Hi::TYPES +# => { entailed_term: "entailedTerm", hotkey: "hotkey", italics: "italics", +# bold: "bold", superscript: "superscript", subscript: "subscript", math: "math" } + +# Create validated elements using constants +note = Tbx::TermNote.new( + type: Tbx::TermNote::TYPES[:part_of_speech], + content: [Tbx::TermNote::VALUES[:part_of_speech][:noun]], +) +---- + +== Supported TBX elements + +=== Structural elements (TBXcoreStructV03.rng) + +[cols="2,3,3",options="header"] +|=== +| Ruby class | TBX element | Schema source + +| `Tbx::Document` | `<tbx>` | Core RNG `<define name="tbx">` +| `Tbx::TbxHeader` | `<tbxHeader>` | Core RNG `<define name="tbxHeader">` +| `Tbx::TextElement` | `<text>` | Core RNG `<define name="text">` +| `Tbx::Body` | `<body>` | Core RNG `<define name="body">` +| `Tbx::Back` | `<back>` | Core RNG `<define name="back">` +| `Tbx::ConceptEntry` | `<conceptEntry>` | Core RNG `<define name="conceptEntry">` +| `Tbx::LangSec` | `<langSec>` | Core RNG `<define name="langSec">` +| `Tbx::TermSec` | `<termSec>` | Core RNG `<define name="termSec">` +| `Tbx::Term` | `<term>` | Core RNG `<define name="term">` +|=== + +=== Header elements (TBXcoreStructV03.rng) + +[cols="2,3,3",options="header"] +|=== +| Ruby class | TBX element | Schema source + +| `Tbx::FileDesc` | `<fileDesc>` | Core RNG `<define name="fileDesc">` +| `Tbx::PublicationStmt` | `<publicationStmt>` | Core RNG `<define name="publicationStmt">` +| `Tbx::TitleStmt` | `<titleStmt>` | Core RNG `<define name="titleStmt">` +| `Tbx::SourceDesc` | `<sourceDesc>` | Core RNG `<define name="sourceDesc">` +| `Tbx::EncodingDesc` | `<encodingDesc>` | Core RNG `<define name="encodingDesc">` +| `Tbx::RevisionDesc` | `<revisionDesc>` | Core RNG `<define name="revisionDesc">` +| `Tbx::Change` | `<change>` | Core RNG `<define name="change">` +| `Tbx::Title` | `<title>` | Core RNG `<define name="title">` +|=== + +=== Data category elements with TYPES constants + +These elements carry a `type` attribute whose permitted values are defined +by the active TBX module composition. The `TYPES` constant on each class +contains the union of all applicable module types. + +==== Admin element + +[cols="1,2,2,3",options="header"] +|=== +| Module | Type value | Content | Source + +| Min | `customerSubset` | string | Min.tbxmd (DC-165) +| Basic | `projectSubset` | string | Basic.tbxmd (DC-406) +| Basic | `source` | string | Basic.tbxmd (DC-471) +| Linguist | `reading` | string | Linguist.tbxmd +|=== + +==== AdminNote element + +[cols="1,2,2,3",options="header"] +|=== +| Module | Type value | Content | Source + +| Linguist | `readingNote` | noteText | Linguist.tbxmd +|=== + +==== Descrip element + +[cols="1,2,2,3",options="header"] +|=== +| Module | Type value | Content | Source + +| Min | `subjectField` | string | Min.tbxmd (DC-489) +| Basic | `context` | noteText | Basic.tbxmd (DC-149) +| Basic | `definition` | noteText | Basic.tbxmd (DC-168) +|=== + +==== TermNote element + +[cols="1,2,2,3",options="header"] +|=== +| Module | Type value | Content | Source + +| Min | `administrativeStatus` | picklist footnote:[admittedTerm-admn-sts, deprecatedTerm-admn-sts, supersededTerm-admn-sts, preferredTerm-admn-sts] | Min.tbxmd (DC-168) +| Min | `partOfSpeech` | picklist footnote:[adjective, noun, other, verb, adverb] | Min.tbxmd (DC-396) +| Basic | `geographicalUsage` | string | Basic.tbxmd (DC-243) +| Basic | `grammaticalGender` | picklist footnote:[masculine, feminine, neuter, other] | Basic.tbxmd (DC-245) +| Basic | `termLocation` | picklist footnote:[18 UI element types: checkBox, comboBox, comboBoxElement, dialogBox, groupBox, informativeMessage, interactiveMessage, menuItem, progressBar, pushButton, radioButton, slider, spinBox, tab, tableText, textBox, toolTip, user-definedType] | Basic.tbxmd (DC-1823) +| Basic | `termType` | picklist footnote:[fullForm, acronym, abbreviation, shortForm, variant, phrase] | Basic.tbxmd (DC-2677) +| Linguist | `grammaticalNumber` | picklist footnote:[singular, plural, dual, mass, otherNumber] | Linguist.tbxmd (DC-251) +| Linguist | `register` | picklist footnote:[colloquialRegister, neutralRegister, technicalRegister, in-houseRegister, bench-levelRegister, slangRegister, vulgarRegister] | Linguist.tbxmd (DC-423) +| Linguist | `transferComment` | string | Linguist.tbxmd (DC-520) +|=== -==== Terminological entries +==== Transac element -`ConceptEntry`, `LangSec`, `TermSec`, `Term` +[cols="1,2,2,3",options="header"] +|=== +| Module | Type value | Values | Source -==== Data categories +| Basic | `transactionType` | picklist footnote:[origination, modification] | Basic.tbxmd (DC-1689) +|=== + +==== TransacNote element + +[cols="1,2,2,3",options="header"] +|=== +| Module | Type value | Content | Source + +| Basic | `responsibility` | string | Basic.tbxmd (DC-451) +|=== -`Admin`, `AdminGrp`, `AdminNote`, `Descrip`, `DescripGrp`, `DescripNote`, -`TermNote`, `TermNoteGrp`, `Ref`, `Xref` +==== Ref element + +[cols="1,2,2,3",options="header"] +|=== +| Module | Type value | Content | Source -==== Transactions +| Basic | `crossReference` | string | Basic.tbxmd (DC-164) +|=== -`Transac`, `TransacGrp`, `TransacNote`, `DateElement` +==== Xref element -==== Header +[cols="1,2,2,3",options="header"] +|=== +| Module | Type value | Content | Source -`FileDesc`, `PublicationStmt`, `TitleStmt`, `SourceDesc`, `EncodingDesc`, -`RevisionDesc`, `Change` +| Min | `externalCrossReference` | string | TBX-Min DCA Schematron +| Basic | `externalCrossReference` | string | Basic.tbxmd (DC-226) +| Basic | `xGraphic` | string | Basic.tbxmd (DC-2920) +|=== -==== Reference objects +==== Hi element (core RNG, not module-specific) -`RefObjectSec`, `RefObject`, `ItemSet`, `ItemGrp`, `Item` +[cols="2,3",options="header"] +|=== +| Type value | Description -==== Inline +| `entailedTerm` | Cross-reference to another concept within term text +| `hotkey` | Keyboard shortcut designation +| `italics` | Italic text emphasis +| `bold` | Bold text emphasis +| `superscript` | Superscript text +| `subscript` | Subscript text +| `math` | Mathematical notation +|=== -`Hi`, `Foreign`, `Ec`, `Sc`, `Ph`, `Note`, `P`, `Title` +=== Grouping elements (TBXcoreStructV03.rng) + +[cols="2,3,3",options="header"] +|=== +| Ruby class | TBX element | Schema source + +| `Tbx::AdminGrp` | `<adminGrp>` | Core RNG `<define name="adminGrp">` +| `Tbx::DescripGrp` | `<descripGrp>` | Core RNG `<define name="descripGrp">` +| `Tbx::DescripNote` | `<descripNote>` | Core RNG `<define name="descripNote">` +| `Tbx::TermNoteGrp` | `<termNoteGrp>` | Core RNG `<define name="termNoteGrp">` +| `Tbx::TransacGrp` | `<transacGrp>` | Core RNG `<define name="transacGrp">` +| `Tbx::TransacNote` | `<transacNote>` | Core RNG `<define name="transacNote">` +| `Tbx::DateElement` | `<date>` | Core RNG `<define name="date">` +|=== + +=== TermComp elements (TermComp-namespace.rng) + +[cols="2,3,3",options="header"] +|=== +| Ruby class | TBX element | Schema source + +| `Tbx::TermCompSec` | `<termCompSec>` | TermComp-namespace.rng `<define name="termCompSec">` +| `Tbx::TermCompGrp` | `<termCompGrp>` | TermComp-namespace.rng `<define name="termCompGrp">` +| `Tbx::TermComp` | `<termComp>` | TermComp-namespace.rng `<define name="termComp">` +|=== + +`Tbx::TermCompSec::TYPES` defines 5 decomposition types: +`hyphenation`, `lemma`, `morphologicalElement`, `syllabification`, `termElement`. + +=== Reference object elements (TBXcoreStructV03.rng) + +[cols="2,3,3",options="header"] +|=== +| Ruby class | TBX element | Schema source + +| `Tbx::RefObjectSec` | `<refObjectSec>` | Core RNG `<define name="refObjectSec">` +| `Tbx::RefObject` | `<refObject>` | Core RNG `<define name="refObject">` +| `Tbx::ItemSet` | `<itemSet>` | Core RNG `<define name="itemSet">` +| `Tbx::ItemGrp` | `<itemGrp>` | Core RNG `<define name="itemGrp">` +| `Tbx::Item` | `<item>` | Core RNG `<define name="item">` +|=== + +=== Inline and text elements (TBXcoreStructV03.rng) + +[cols="2,3,3",options="header"] +|=== +| Ruby class | TBX element | Schema source + +| `Tbx::Hi` | `<hi>` | Core RNG `<define name="hi">` +| `Tbx::Foreign` | `<foreign>` | Core RNG `<define name="foreign">` +| `Tbx::Ec` | `<ec>` | Core RNG `<define name="ec">` +| `Tbx::Sc` | `<sc>` | Core RNG `<define name="sc">` +| `Tbx::Ph` | `<ph>` | Core RNG `<define name="ph">` +| `Tbx::Note` | `<note>` | Core RNG `<define name="note">` +| `Tbx::P` | `<p>` | Core RNG `<define name="p">` +|=== + +== Module architecture + +TBX modules define sets of data categories. Dialects compose modules to +determine which `@type` values are permitted on each element. + +=== Modules and dialects + +[cols="1,4,3",options="header"] +|=== +| Module | Dialects that include it | Source files + +| Min | TBX-Min, TBX-Basic, TBX-Core, TBX-Linguist | `Min.tbxmd`, `Min.rng`, `Min.sch` +| Basic | TBX-Basic, TBX-Linguist | `Basic.tbxmd`, `Basic.rng`, `Basic.sch` +| Linguist | TBX-Linguist | `Linguist.tbxmd`, `Linguist.rng`, `Linguist.sch` +| TermComp | (add-on for any dialect) | `TermComp-namespace.rng` +| Core | TBX-Core | `TBXcoreStructV03.rng` +|=== + +=== Ruby module constants + +[cols="2,3,5",options="header"] +|=== +| Ruby module | Constants | Source schema + +| `Tbx::Modules::Min` | `ADMIN_TYPES`, `DESCRIP_TYPES`, `TERM_NOTE_TYPES`, `TERM_NOTE_VALUES`, `XREF_TYPES` | Min.tbxmd +| `Tbx::Modules::Basic` | `ADMIN_TYPES`, `DESCRIP_TYPES`, `TERM_NOTE_TYPES`, `TERM_NOTE_VALUES`, `REF_TYPES`, `XREF_TYPES`, `TRANSAC_TYPES`, `TRANSAC_VALUES`, `TRANSAC_NOTE_TYPES` | Basic.tbxmd +| `Tbx::Modules::Linguist` | `ADMIN_TYPES`, `ADMIN_NOTE_TYPES`, `TERM_NOTE_TYPES`, `TERM_NOTE_VALUES` | Linguist.tbxmd +| `Tbx::Modules::CoreTypes` | `HI_TYPES` | TBXcoreStructV03.rng +|=== + +Element classes compose these via `merge`: + +[cols="2,3",options="header"] +|=== +| Element class | TYPES composition + +| `Tbx::Admin` | Min::ADMIN_TYPES + Basic::ADMIN_TYPES + Linguist::ADMIN_TYPES +| `Tbx::AdminNote` | Linguist::ADMIN_NOTE_TYPES +| `Tbx::Descrip` | Min::DESCRIP_TYPES + Basic::DESCRIP_TYPES +| `Tbx::TermNote` | Min::TERM_NOTE_TYPES + Basic::TERM_NOTE_TYPES + Linguist::TERM_NOTE_TYPES +| `Tbx::Ref` | Basic::REF_TYPES +| `Tbx::Xref` | Min::XREF_TYPES + Basic::XREF_TYPES +| `Tbx::Transac` | Basic::TRANSAC_TYPES +| `Tbx::TransacNote` | Basic::TRANSAC_NOTE_TYPES +| `Tbx::Hi` | CoreTypes::HI_TYPES +| `Tbx::TermCompSec` | (self-contained: hyphenation, lemma, morphologicalElement, syllabification, termElement) +|=== + +=== Shared concern + +`Tbx::DataElement` is a module that injects common attributes (id, lang, +target, datatype, type, content) via `self.included(base)`. +`Tbx::DataElement::InlineContent` adds inline child attributes (hi, ec, +foreign, ph, sc) for elements with `entity.noteText` content. + +[cols="2,2",options="header"] +|=== +| Element classes | Includes InlineContent? +| `Admin`, `Descrip`, `TermNote` | Yes (entity.noteText content) +| `AdminNote`, `DescripNote`, `TransacNote`, `Transac`, `Ref` | No (plain text only per RNG) +|=== + +== Schema source audit + +Every element class in `lib/tbx/` has YARD documentation tracing it to its +schema source. The authoritative sources are: + +[cols="2,5",options="header"] +|=== +| Source file | Defines + +| `TBXcoreStructV03.rng` | All structural elements, attributes, content models, and `hi` type values +| `Min.tbxmd` | Min module data categories: customerSubset, subjectField, administrativeStatus, partOfSpeech, externalCrossReference +| `Basic.tbxmd` | Basic module data categories: projectSubset, source, context, definition, geographicalUsage, grammaticalGender, termLocation, termType, crossReference, externalCrossReference, xGraphic, transactionType, responsibility +| `Linguist.tbxmd` | Linguist module data categories: reading, readingNote, grammaticalNumber, register, transferComment +| `TermComp-namespace.rng` | TermComp elements (termComp, termCompGrp, termCompSec) and type values +| `TBX-Basic_DCA.sch` | TBX-Basic DCA Schematron: permitted `@type` values, picklist value constraints, level constraints +| `TBX-Min_DCA.sch` | TBX-Min DCA Schematron +| `TBX-Linguist_DCA.sch` | TBX-Linguist DCA Schematron +| `TBX-Core.sch` | TBX-Core Schematron +| `Basic.rng` / `Min.rng` / `Linguist.rng` | Module-level structural extensions +| `Basic.sch` / `Min.sch` / `Linguist.sch` | Module-level Schematron rules +|=== + +== Reference documentation + +The `reference-docs/` directory contains official TBX schema, dialect, and +module files from https://ltac-global.org[LTAC Global]. See +link:reference-docs/README.adoc[reference-docs/README.adoc] for a complete +inventory with source repository links. + +=== Official LTAC-Global repositories + +|=== +| Repository | Description + +| https://github.com/LTAC-Global/TBX_core_module[TBX_core_module] +| Core structural schema (`TBXcoreStructV03.rng`) + +| https://github.com/LTAC-Global/TBX_min_module[TBX_min_module] +| Min module data categories (RNG, Schematron, `.tbxmd`) + +| https://github.com/LTAC-Global/TBX_basic_module[TBX_basic_module] +| Basic module data categories (RNG, Schematron, `.tbxmd`) + +| https://github.com/LTAC-Global/TBX_linguist_module[TBX_linguist_module] +| Linguist module data categories (RNG, Schematron, `.tbxmd`) + +| https://github.com/LTAC-Global/TBX_termComp_module[TBX_termComp_module] +| Term composition module (namespace RNG) + +| https://github.com/LTAC-Global/TBX_module_description_xml[TBX_module_description_xml] +| `.tbxmd` format schema (`tbxmd.rng`) + +| https://github.com/LTAC-Global/TBX-Min_dialect[TBX-Min_dialect] +| TBX-Min dialect (DCA + DCT Schematron, NVDL) + +| https://github.com/LTAC-Global/TBX-Basic_dialect[TBX-Basic_dialect] +| TBX-Basic dialect (DCA + DCT Schematron, bundled modules) + +| https://github.com/LTAC-Global/TBX-Core_dialect[TBX-Core_dialect] +| TBX-Core dialect (integrated RNG, Schematron) + +| https://github.com/LTAC-Global/TBX-Linguist_dialect[TBX-Linguist_dialect] +| TBX-Linguist dialect (DCA + DCT Schematron, integrated RNG) + +| https://github.com/LTAC-Global/TBX-Basic_ImplementationGuide[TBX-Basic_ImplementationGuide] +| TBX-Basic implementation guide + +| https://github.com/LTAC-Global/TBX_test_files[TBX_test_files] +| Official TBX test fixture files +|=== == Test data Test fixtures are sourced from the https://github.com/LTAC-Global/TBX_test_files[TBX_test_files] repository -maintained by https://ltac-global.org[LTAC Global], and from the TBX-Basic -dialect schemas included in `reference-docs/`. +maintained by https://ltac-global.org[LTAC Global], and from the dialect +schemas and example files in `reference-docs/`. == Development @@ -150,6 +492,10 @@ bundle exec rake This gem is developed, maintained and funded by https://www.ribose.com[Ribose Inc.] +TBX schema, dialect, and module reference files are maintained by +https://ltac-global.org[LTAC Global] and sourced from the +https://github.com/LTAC-Global[LTAC-Global GitHub organization]. + == License The gem is available as open source under the terms of the diff --git a/lib/tbx.rb b/lib/tbx.rb index 934c550..18831a5 100644 --- a/lib/tbx.rb +++ b/lib/tbx.rb @@ -4,6 +4,13 @@ require_relative "tbx/version" module Tbx + module Modules + autoload :Min, "#{__dir__}/tbx/modules/min" + autoload :Basic, "#{__dir__}/tbx/modules/basic" + autoload :Linguist, "#{__dir__}/tbx/modules/linguist" + autoload :CoreTypes, "#{__dir__}/tbx/modules/core_types" + end + autoload :Namespace, "#{__dir__}/tbx/namespace" # Inline elements @@ -18,6 +25,9 @@ module Tbx autoload :P, "#{__dir__}/tbx/p" autoload :Title, "#{__dir__}/tbx/title" + # Shared concerns + autoload :DataElement, "#{__dir__}/tbx/data_element" + # Data elements autoload :Admin, "#{__dir__}/tbx/admin" autoload :AdminGrp, "#{__dir__}/tbx/admin_grp" @@ -45,6 +55,9 @@ module Tbx # Structural elements autoload :Term, "#{__dir__}/tbx/term" + autoload :TermComp, "#{__dir__}/tbx/term_comp" + autoload :TermCompGrp, "#{__dir__}/tbx/term_comp_grp" + autoload :TermCompSec, "#{__dir__}/tbx/term_comp_sec" autoload :TermSec, "#{__dir__}/tbx/term_sec" autoload :LangSec, "#{__dir__}/tbx/lang_sec" autoload :ConceptEntry, "#{__dir__}/tbx/concept_entry" diff --git a/lib/tbx/admin.rb b/lib/tbx/admin.rb index 4acc9e7..604845a 100644 --- a/lib/tbx/admin.rb +++ b/lib/tbx/admin.rb @@ -1,18 +1,31 @@ # frozen_string_literal: true module Tbx + # Administrative data category element `<admin>`. + # + # Carries administrative metadata about a terminological entry, such as + # customer subset classification, project association, source attribution, + # and pronunciation readings. + # + # Permitted `type` values (composed from all modules): + # + # * Min module: `customerSubset` — entry subset (DC-165) + # * Basic module: `projectSubset` — project-specific entry subset (DC-406), + # `source` — origin of information (DC-471) + # * Linguist module: `reading` — pronunciation or reading of a term + # + # Content model: `entity.noteText` (mixed text + inline elements hi, ec, + # foreign, ph, sc). + # + # Schema source: TBXcoreStructV03.rng `<define name="admin">`; + # data categories: Min.tbxmd, Basic.tbxmd, Linguist.tbxmd. class Admin < Lutaml::Model::Serializable - attribute :id, :string - attribute :lang, Lutaml::Xml::W3c::XmlLangType - attribute :target, :string - attribute :datatype, :string - attribute :type, :string - attribute :content, :string, collection: true - attribute :hi, ::Tbx::Hi, collection: true - attribute :ec, ::Tbx::Ec, collection: true - attribute :foreign, ::Tbx::Foreign, collection: true - attribute :ph, ::Tbx::Ph, collection: true - attribute :sc, ::Tbx::Sc, collection: true + include Tbx::DataElement + include Tbx::DataElement::InlineContent + + TYPES = Modules::Min::ADMIN_TYPES + .merge(Modules::Basic::ADMIN_TYPES) + .merge(Modules::Linguist::ADMIN_TYPES).freeze xml do root "admin" diff --git a/lib/tbx/admin_grp.rb b/lib/tbx/admin_grp.rb index c835ba6..fbf935e 100644 --- a/lib/tbx/admin_grp.rb +++ b/lib/tbx/admin_grp.rb @@ -1,6 +1,11 @@ # frozen_string_literal: true module Tbx + # Groups an `<admin>` element with its associated notes and references. + # + # Children: `admin` (required), then adminNote, note, ref, xref. + # + # Schema source: TBXcoreStructV03.rng `<define name="adminGrp">` class AdminGrp < Lutaml::Model::Serializable attribute :id, :string attribute :admin, ::Tbx::Admin diff --git a/lib/tbx/admin_note.rb b/lib/tbx/admin_note.rb index 32523a2..15adde9 100644 --- a/lib/tbx/admin_note.rb +++ b/lib/tbx/admin_note.rb @@ -1,13 +1,21 @@ # frozen_string_literal: true module Tbx + # Administrative note element `<adminNote>`. + # + # Provides notes about administrative data. Content is plain text only + # (no inline elements per the core RNG). + # + # Permitted `type` values: + # + # * Linguist module: `readingNote` — note about a term's reading/pronunciation + # + # Schema source: TBXcoreStructV03.rng `<define name="adminNote">`; + # data category: Linguist.tbxmd. class AdminNote < Lutaml::Model::Serializable - attribute :id, :string - attribute :lang, Lutaml::Xml::W3c::XmlLangType - attribute :target, :string - attribute :datatype, :string - attribute :type, :string - attribute :content, :string, collection: true + include Tbx::DataElement + + TYPES = Modules::Linguist::ADMIN_NOTE_TYPES.freeze xml do root "adminNote" diff --git a/lib/tbx/back.rb b/lib/tbx/back.rb index b64967a..39cf586 100644 --- a/lib/tbx/back.rb +++ b/lib/tbx/back.rb @@ -1,6 +1,11 @@ # frozen_string_literal: true module Tbx + # Back matter `<back>` containing reference object sections. + # + # Used for managing picklists and external references. + # + # Schema source: TBXcoreStructV03.rng `<define name="back">` class Back < Lutaml::Model::Serializable attribute :id, :string attribute :ref_object_sec, ::Tbx::RefObjectSec, collection: true diff --git a/lib/tbx/body.rb b/lib/tbx/body.rb index 785ee7d..67a60be 100644 --- a/lib/tbx/body.rb +++ b/lib/tbx/body.rb @@ -1,6 +1,9 @@ # frozen_string_literal: true module Tbx + # Body element `<body>` containing all concept entries. + # + # Schema source: TBXcoreStructV03.rng `<define name="body">` class Body < Lutaml::Model::Serializable attribute :id, :string attribute :concept_entry, ::Tbx::ConceptEntry, collection: true diff --git a/lib/tbx/change.rb b/lib/tbx/change.rb index 6fe7c3c..629d840 100644 --- a/lib/tbx/change.rb +++ b/lib/tbx/change.rb @@ -1,6 +1,12 @@ # frozen_string_literal: true module Tbx + # A single change record in the revision history `<change>`. + # + # Each change record contains one or more paragraph elements describing + # what changed and when. + # + # Schema source: TBXcoreStructV03.rng `<define name="change">` class Change < Lutaml::Model::Serializable attribute :id, :string attribute :lang, Lutaml::Xml::W3c::XmlLangType diff --git a/lib/tbx/concept_entry.rb b/lib/tbx/concept_entry.rb index 4354866..90d64d7 100644 --- a/lib/tbx/concept_entry.rb +++ b/lib/tbx/concept_entry.rb @@ -1,6 +1,16 @@ # frozen_string_literal: true module Tbx + # A single concept entry `<conceptEntry>`. + # + # Represents a concept in the terminology collection. The `id` attribute + # is required and must be unique within the document. + # + # Permitted children are defined by the `entity.auxInfo` pattern: + # admin, adminGrp, descrip, descripGrp, note, ref, transacGrp, xref, + # followed by one or more langSec elements. + # + # Schema source: TBXcoreStructV03.rng `<define name="conceptEntry">` class ConceptEntry < Lutaml::Model::Serializable attribute :id, :string attribute :admin, ::Tbx::Admin, collection: true diff --git a/lib/tbx/data_element.rb b/lib/tbx/data_element.rb new file mode 100644 index 0000000..7498ae1 --- /dev/null +++ b/lib/tbx/data_element.rb @@ -0,0 +1,50 @@ +# frozen_string_literal: true + +module Tbx + # Shared attribute declarations for TBX data-category elements. + # + # Injects the common attributes defined by the `IDLangTgtDtyp` attribute + # class + `type` + text content pattern from TBXcoreStructV03.rng. + # + # @example Usage in a data-category element + # class Admin < Lutaml::Model::Serializable + # include Tbx::DataElement + # include Tbx::DataElement::InlineContent + # + # xml do + # root "admin" + # ... + # end + # end + module DataElement + def self.included(base) + base.class_eval do + attribute :id, :string + attribute :lang, Lutaml::Xml::W3c::XmlLangType + attribute :target, :string + attribute :datatype, :string + attribute :type, :string + attribute :content, :string, collection: true + end + end + + # Inline child element attributes for data-category elements that + # support mixed content per the `entity.noteText` pattern in + # TBXcoreStructV03.rng. + # + # Included by: Admin, Descrip, TermNote (elements with noteText content). + # NOT included by: AdminNote, DescripNote, TransacNote, Transac, Ref + # (plain text only per RNG). + module InlineContent + def self.included(base) + base.class_eval do + attribute :hi, ::Tbx::Hi, collection: true + attribute :ec, ::Tbx::Ec, collection: true + attribute :foreign, ::Tbx::Foreign, collection: true + attribute :ph, ::Tbx::Ph, collection: true + attribute :sc, ::Tbx::Sc, collection: true + end + end + end + end +end diff --git a/lib/tbx/date.rb b/lib/tbx/date.rb index 741f832..176d39a 100644 --- a/lib/tbx/date.rb +++ b/lib/tbx/date.rb @@ -1,6 +1,12 @@ # frozen_string_literal: true module Tbx + # Date element `<date>`. + # + # Records when a transaction occurred. Content must be a valid XML Schema + # `date` (YYYY-MM-DD) or `dateTime` (YYYY-MM-DDThh:mm:ss) value. + # + # Schema source: TBXcoreStructV03.rng `<define name="date">` class DateElement < Lutaml::Model::Serializable attribute :id, :string attribute :content, :string diff --git a/lib/tbx/descrip.rb b/lib/tbx/descrip.rb index 45b2e8e..1d39bc9 100644 --- a/lib/tbx/descrip.rb +++ b/lib/tbx/descrip.rb @@ -1,18 +1,30 @@ # frozen_string_literal: true module Tbx + # Descriptive data category element `<descrip>`. + # + # Carries conceptual and contextual information about a term, including + # definitions, subject field classifications, and usage contexts. + # + # Permitted `type` values (composed from all modules): + # + # * Min module: `subjectField` — field of special knowledge (DC-489), + # level: conceptEntry + # * Basic module: `context` — text illustrating term usage (DC-149), + # level: termSec; `definition` — narrative statement of concept (DC-168), + # level: conceptEntry/langSec + # + # Content model: `entity.noteText` (mixed text + inline elements hi, ec, + # foreign, ph, sc). + # + # Schema source: TBXcoreStructV03.rng `<define name="descrip">`; + # data categories: Min.tbxmd, Basic.tbxmd. class Descrip < Lutaml::Model::Serializable - attribute :id, :string - attribute :lang, Lutaml::Xml::W3c::XmlLangType - attribute :target, :string - attribute :datatype, :string - attribute :type, :string - attribute :content, :string, collection: true - attribute :hi, ::Tbx::Hi, collection: true - attribute :ec, ::Tbx::Ec, collection: true - attribute :foreign, ::Tbx::Foreign, collection: true - attribute :ph, ::Tbx::Ph, collection: true - attribute :sc, ::Tbx::Sc, collection: true + include Tbx::DataElement + include Tbx::DataElement::InlineContent + + TYPES = Modules::Min::DESCRIP_TYPES + .merge(Modules::Basic::DESCRIP_TYPES).freeze xml do root "descrip" diff --git a/lib/tbx/descrip_grp.rb b/lib/tbx/descrip_grp.rb index 9567c47..fb26121 100644 --- a/lib/tbx/descrip_grp.rb +++ b/lib/tbx/descrip_grp.rb @@ -1,6 +1,13 @@ # frozen_string_literal: true module Tbx + # Groups a `<descrip>` element with its administrative data, notes, and + # source references. + # + # Commonly used to associate a `source` admin with a `definition` descrip, + # providing provenance for descriptive data. + # + # Schema source: TBXcoreStructV03.rng `<define name="descripGrp">` class DescripGrp < Lutaml::Model::Serializable attribute :id, :string attribute :descrip, ::Tbx::Descrip diff --git a/lib/tbx/descrip_note.rb b/lib/tbx/descrip_note.rb index facb1a3..15416c7 100644 --- a/lib/tbx/descrip_note.rb +++ b/lib/tbx/descrip_note.rb @@ -1,13 +1,13 @@ # frozen_string_literal: true module Tbx + # Note element associated with a `<descrip>` description. + # + # Content is plain text only (no inline elements per the core RNG). + # + # Schema source: TBXcoreStructV03.rng `<define name="descripNote">` class DescripNote < Lutaml::Model::Serializable - attribute :id, :string - attribute :lang, Lutaml::Xml::W3c::XmlLangType - attribute :target, :string - attribute :datatype, :string - attribute :type, :string - attribute :content, :string, collection: true + include Tbx::DataElement xml do root "descripNote" diff --git a/lib/tbx/document.rb b/lib/tbx/document.rb index 0dc61c5..ae82e76 100644 --- a/lib/tbx/document.rb +++ b/lib/tbx/document.rb @@ -1,6 +1,18 @@ # frozen_string_literal: true module Tbx + # Root element of a TBX (Termbase Exchange) document per ISO 30042:2019. + # + # The `type` attribute declares the dialect (e.g. "TBX-Basic", "TBX-Min", + # "TBX-Core", "TBX-Linguist"), and `style` declares the serialization + # style ("dca" for Data Category Archive or "dct" for Data Category Tagging). + # + # @example Parsing a TBX file + # doc = Tbx::Document.from_xml(File.read("glossary.tbx")) + # doc.type # => "TBX-Basic" + # doc.style # => "dca" + # + # Schema source: TBXcoreStructV03.rng `<define name="tbx">` class Document < Lutaml::Model::Serializable attribute :lang, Lutaml::Xml::W3c::XmlLangType attribute :type, :string diff --git a/lib/tbx/ec.rb b/lib/tbx/ec.rb index c67ee4d..54d7dae 100644 --- a/lib/tbx/ec.rb +++ b/lib/tbx/ec.rb @@ -1,6 +1,22 @@ # frozen_string_literal: true module Tbx + # XLIFF inline end-code marker `<ec>`. + # + # Used for representing inline formatting codes from source formats. + # Paired with `<sc>` via the `startRef` attribute. + # + # Attributes: + # * `startRef` (IDREF) — references the id of the corresponding `<sc>` + # * `isolated` (yes/no) — whether this code is isolated + # * `disp` — display text + # * `equiv` — equivalent text + # * `id` — unique identifier + # * `type` (fmt, ui, quote, link, image, other) — code type + # * `subtype` — sub-classification + # * `target` — target reference + # + # Schema source: TBXcoreStructV03.rng `<define name="ec">` class Ec < Lutaml::Model::Serializable attribute :start_ref, :string attribute :isolated, :string diff --git a/lib/tbx/encoding_desc.rb b/lib/tbx/encoding_desc.rb index a505e80..98ef505 100644 --- a/lib/tbx/encoding_desc.rb +++ b/lib/tbx/encoding_desc.rb @@ -1,6 +1,9 @@ # frozen_string_literal: true module Tbx + # Encoding description `<encodingDesc>`. + # + # Schema source: TBXcoreStructV03.rng `<define name="encodingDesc">` class EncodingDesc < Lutaml::Model::Serializable attribute :id, :string attribute :p, ::Tbx::P, collection: true diff --git a/lib/tbx/file_desc.rb b/lib/tbx/file_desc.rb index 73fd7bb..24295d3 100644 --- a/lib/tbx/file_desc.rb +++ b/lib/tbx/file_desc.rb @@ -1,6 +1,12 @@ # frozen_string_literal: true module Tbx + # File description `<fileDesc>`. + # + # Contains file-level metadata including publication statement, title, + # and source description. + # + # Schema source: TBXcoreStructV03.rng `<define name="fileDesc">` class FileDesc < Lutaml::Model::Serializable attribute :id, :string attribute :publication_stmt, ::Tbx::PublicationStmt diff --git a/lib/tbx/foreign.rb b/lib/tbx/foreign.rb index cf2afc4..e2606bf 100644 --- a/lib/tbx/foreign.rb +++ b/lib/tbx/foreign.rb @@ -1,6 +1,12 @@ # frozen_string_literal: true module Tbx + # Foreign-language text element `<foreign>`. + # + # Marks text in a foreign language. The `xml:lang` attribute indicates + # the language. Content model: `entity.noteText` (mixed text + inline + # elements). + # Schema source: TBXcoreStructV03.rng `<define name="foreign">` class Foreign < Lutaml::Model::Serializable attribute :id, :string attribute :lang, Lutaml::Xml::W3c::XmlLangType diff --git a/lib/tbx/hi.rb b/lib/tbx/hi.rb index 2510ad7..a61c99a 100644 --- a/lib/tbx/hi.rb +++ b/lib/tbx/hi.rb @@ -1,7 +1,25 @@ # frozen_string_literal: true module Tbx + # Inline highlighting element `<hi>`. + # + # Used within term, note, and other text content to mark up special text + # ranges. The `entailedTerm` type with `target` attribute creates inline + # cross-references to other concepts. + # + # Permitted `type` values (from Core RNG): + # + # * `entailedTerm` — cross-reference to another concept within term text + # * `hotkey` — keyboard shortcut designation + # * `italics` — italic text emphasis + # * `bold` — bold text emphasis + # * `superscript` — superscript text + # * `subscript` — subscript text + # * `math` — mathematical notation + # + # Schema source: TBXcoreStructV03.rng `<define name="hi">` class Hi < Lutaml::Model::Serializable + TYPES = Modules::CoreTypes::HI_TYPES.freeze attribute :target, :string attribute :type, :string attribute :content, :string, collection: true diff --git a/lib/tbx/item.rb b/lib/tbx/item.rb index 6cd0cad..9e322a9 100644 --- a/lib/tbx/item.rb +++ b/lib/tbx/item.rb @@ -1,6 +1,12 @@ # frozen_string_literal: true module Tbx + # A single picklist value item `<item>`. + # + # Content model: `entity.noteText` (mixed text + inline elements: + # hi, ec, foreign, ph, sc). + # + # Schema source: TBXcoreStructV03.rng `<define name="item">` class Item < Lutaml::Model::Serializable attribute :id, :string attribute :type, :string diff --git a/lib/tbx/item_grp.rb b/lib/tbx/item_grp.rb index 7cc2c02..b2117f5 100644 --- a/lib/tbx/item_grp.rb +++ b/lib/tbx/item_grp.rb @@ -1,6 +1,12 @@ # frozen_string_literal: true module Tbx + # Item group `<itemGrp>` associating a picklist item with administrative data. + # + # Groups an `item` with its associated administrative data, notes, + # references, and transaction records. + # + # Schema source: TBXcoreStructV03.rng `<define name="itemGrp">` class ItemGrp < Lutaml::Model::Serializable attribute :id, :string attribute :item, ::Tbx::Item diff --git a/lib/tbx/item_set.rb b/lib/tbx/item_set.rb index 4e5de97..644def4 100644 --- a/lib/tbx/item_set.rb +++ b/lib/tbx/item_set.rb @@ -1,6 +1,12 @@ # frozen_string_literal: true module Tbx + # A set of items forming a picklist `<itemSet>`. + # + # Contains `itemGrp` or `item` children that enumerate individual + # picklist values. + # + # Schema source: TBXcoreStructV03.rng `<define name="itemSet">` class ItemSet < Lutaml::Model::Serializable attribute :id, :string attribute :type, :string diff --git a/lib/tbx/lang_sec.rb b/lib/tbx/lang_sec.rb index 633773e..926431d 100644 --- a/lib/tbx/lang_sec.rb +++ b/lib/tbx/lang_sec.rb @@ -1,6 +1,12 @@ # frozen_string_literal: true module Tbx + # Language section `<langSec>`. + # + # Groups all term-level data for a single language within a concept entry. + # The `xml:lang` attribute is required and specifies the language. + # + # Schema source: TBXcoreStructV03.rng `<define name="langSec">` class LangSec < Lutaml::Model::Serializable attribute :lang, Lutaml::Xml::W3c::XmlLangType attribute :admin, ::Tbx::Admin, collection: true diff --git a/lib/tbx/modules/basic.rb b/lib/tbx/modules/basic.rb new file mode 100644 index 0000000..e3f10c7 --- /dev/null +++ b/lib/tbx/modules/basic.rb @@ -0,0 +1,92 @@ +# frozen_string_literal: true + +module Tbx + module Modules + # Data category definitions for the TBX-Basic module. + # + # TBX-Basic extends Min with additional data categories for standard + # terminology exchange including definitions, context, term types, + # and transaction tracking. + # + # Source: Basic.tbxmd, Basic.rng, Basic.sch + module Basic + ADMIN_TYPES = { + project_subset: "projectSubset", + source: "source", + }.freeze + + DESCRIP_TYPES = { + context: "context", + definition: "definition", + }.freeze + + TERM_NOTE_TYPES = { + geographical_usage: "geographicalUsage", + grammatical_gender: "grammaticalGender", + term_location: "termLocation", + term_type: "termType", + }.freeze + + TERM_NOTE_VALUES = { + grammatical_gender: { + masculine: "masculine", + feminine: "feminine", + neuter: "neuter", + other: "other", + }.freeze, + term_location: { + check_box: "checkBox", + combo_box: "comboBox", + combo_box_element: "comboBoxElement", + dialog_box: "dialogBox", + group_box: "groupBox", + informative_message: "informativeMessage", + interactive_message: "interactiveMessage", + menu_item: "menuItem", + progress_bar: "progressBar", + push_button: "pushButton", + radio_button: "radioButton", + slider: "slider", + spin_box: "spinBox", + tab: "tab", + table_text: "tableText", + text_box: "textBox", + tool_tip: "toolTip", + user_defined_type: "user-definedType", + }.freeze, + term_type: { + full_form: "fullForm", + acronym: "acronym", + abbreviation: "abbreviation", + short_form: "shortForm", + variant: "variant", + phrase: "phrase", + }.freeze, + }.freeze + + REF_TYPES = { + cross_reference: "crossReference", + }.freeze + + XREF_TYPES = { + external_cross_reference: "externalCrossReference", + x_graphic: "xGraphic", + }.freeze + + TRANSAC_TYPES = { + transaction_type: "transactionType", + }.freeze + + TRANSAC_VALUES = { + transaction_type: { + origination: "origination", + modification: "modification", + }.freeze, + }.freeze + + TRANSAC_NOTE_TYPES = { + responsibility: "responsibility", + }.freeze + end + end +end diff --git a/lib/tbx/modules/core_types.rb b/lib/tbx/modules/core_types.rb new file mode 100644 index 0000000..134df0c --- /dev/null +++ b/lib/tbx/modules/core_types.rb @@ -0,0 +1,23 @@ +# frozen_string_literal: true + +module Tbx + module Modules + # Data category definitions from the TBX core RNG schema. + # + # These types are not module-specific; they are defined directly in + # TBXcoreStructV03.rng and apply to all dialects. + module CoreTypes + # Permitted `<hi>` element type values per TBXcoreStructV03.rng + # `<define name="hi">`. + HI_TYPES = { + entailed_term: "entailedTerm", + hotkey: "hotkey", + italics: "italics", + bold: "bold", + superscript: "superscript", + subscript: "subscript", + math: "math", + }.freeze + end + end +end diff --git a/lib/tbx/modules/linguist.rb b/lib/tbx/modules/linguist.rb new file mode 100644 index 0000000..e41bf3b --- /dev/null +++ b/lib/tbx/modules/linguist.rb @@ -0,0 +1,46 @@ +# frozen_string_literal: true + +module Tbx + module Modules + # Data category definitions for the TBX-Linguist module. + # + # TBX-Linguist extends Basic with additional linguistic data categories + # including grammatical number, register, and transfer comments. + # + # Source: Linguist.tbxmd, Linguist.rng, Linguist.sch + module Linguist + ADMIN_TYPES = { + reading: "reading", + }.freeze + + ADMIN_NOTE_TYPES = { + reading_note: "readingNote", + }.freeze + + TERM_NOTE_TYPES = { + grammatical_number: "grammaticalNumber", + register: "register", + transfer_comment: "transferComment", + }.freeze + + TERM_NOTE_VALUES = { + grammatical_number: { + singular: "singular", + plural: "plural", + dual: "dual", + mass: "mass", + other_number: "otherNumber", + }.freeze, + register: { + colloquial: "colloquialRegister", + neutral: "neutralRegister", + technical: "technicalRegister", + in_house: "in-houseRegister", + bench_level: "bench-levelRegister", + slang: "slangRegister", + vulgar: "vulgarRegister", + }.freeze, + }.freeze + end + end +end diff --git a/lib/tbx/modules/min.rb b/lib/tbx/modules/min.rb new file mode 100644 index 0000000..ac03ba2 --- /dev/null +++ b/lib/tbx/modules/min.rb @@ -0,0 +1,46 @@ +# frozen_string_literal: true + +module Tbx + module Modules + # Data category definitions for the TBX-Min module. + # + # TBX-Min provides a minimal set of data categories for simple + # terminology exchange. + # + # Source: Min.tbxmd, Min.rng, Min.sch + module Min + ADMIN_TYPES = { + customer_subset: "customerSubset", + }.freeze + + DESCRIP_TYPES = { + subject_field: "subjectField", + }.freeze + + TERM_NOTE_TYPES = { + administrative_status: "administrativeStatus", + part_of_speech: "partOfSpeech", + }.freeze + + TERM_NOTE_VALUES = { + administrative_status: { + admitted_term: "admittedTerm-admn-sts", + deprecated_term: "deprecatedTerm-admn-sts", + superseded_term: "supersededTerm-admn-sts", + preferred_term: "preferredTerm-admn-sts", + }.freeze, + part_of_speech: { + adjective: "adjective", + noun: "noun", + other: "other", + verb: "verb", + adverb: "adverb", + }.freeze, + }.freeze + + XREF_TYPES = { + external_cross_reference: "externalCrossReference", + }.freeze + end + end +end diff --git a/lib/tbx/namespace.rb b/lib/tbx/namespace.rb index afb355e..50f47b9 100644 --- a/lib/tbx/namespace.rb +++ b/lib/tbx/namespace.rb @@ -1,6 +1,11 @@ # frozen_string_literal: true module Tbx + # XML namespace for TBX elements per ISO 30042:2019. + # + # URI: `urn:iso:std:iso:30042:ed-2` + # + # All TBX structural elements use this namespace. class Namespace < Lutaml::Xml::Namespace uri "urn:iso:std:iso:30042:ed-2" end diff --git a/lib/tbx/note.rb b/lib/tbx/note.rb index 4401e2d..766be29 100644 --- a/lib/tbx/note.rb +++ b/lib/tbx/note.rb @@ -1,6 +1,15 @@ # frozen_string_literal: true module Tbx + # Generic note element `<note>`. + # + # Provides supplementary information at conceptEntry, langSec, termSec, + # and various group levels. + # + # Content model: `entity.noteText` (mixed text + inline elements hi, ec, + # foreign, ph, sc). + # + # Schema source: TBXcoreStructV03.rng `<define name="note">` class Note < Lutaml::Model::Serializable attribute :id, :string attribute :lang, Lutaml::Xml::W3c::XmlLangType diff --git a/lib/tbx/p.rb b/lib/tbx/p.rb index 378dab6..7c4088e 100644 --- a/lib/tbx/p.rb +++ b/lib/tbx/p.rb @@ -1,6 +1,15 @@ # frozen_string_literal: true module Tbx + # Paragraph element `<p>`. + # + # Used for prose text in header contexts (publicationStmt, sourceDesc, + # encodingDesc, change). + # + # Content model: `entity.noteText` (mixed text + inline elements hi, ec, + # foreign, ph, sc). + # + # Schema source: TBXcoreStructV03.rng `<define name="p">` class P < Lutaml::Model::Serializable attribute :id, :string attribute :lang, Lutaml::Xml::W3c::XmlLangType diff --git a/lib/tbx/ph.rb b/lib/tbx/ph.rb index 75ac750..817a076 100644 --- a/lib/tbx/ph.rb +++ b/lib/tbx/ph.rb @@ -1,6 +1,12 @@ # frozen_string_literal: true module Tbx + # XLIFF inline placeholder `<ph>`. + # + # Represents a code that does not have a distinct start and end. + # Empty element with optional `type` attribute. + # + # Schema source: TBXcoreStructV03.rng `<define name="ph">` class Ph < Lutaml::Model::Serializable attribute :type, :string diff --git a/lib/tbx/publication_stmt.rb b/lib/tbx/publication_stmt.rb index 2aac4d0..d4153b4 100644 --- a/lib/tbx/publication_stmt.rb +++ b/lib/tbx/publication_stmt.rb @@ -1,6 +1,9 @@ # frozen_string_literal: true module Tbx + # Publication statement `<publicationStmt>`. + # + # Schema source: TBXcoreStructV03.rng `<define name="publicationStmt">` class PublicationStmt < Lutaml::Model::Serializable attribute :id, :string attribute :p, ::Tbx::P, collection: true diff --git a/lib/tbx/ref.rb b/lib/tbx/ref.rb index d1e0f81..28453f7 100644 --- a/lib/tbx/ref.rb +++ b/lib/tbx/ref.rb @@ -1,13 +1,24 @@ # frozen_string_literal: true module Tbx + # Internal reference element `<ref>`. + # + # Used for cross-references within the same termbase. The `target` + # attribute holds an IDREF pointing to another element's `id`. + # + # Permitted `type` values: + # + # * Basic module: `crossReference` — reference to another concept entry + # in the same termbase (DC-164), level: conceptEntry/termSec + # + # Content is plain text only (no inline elements per the core RNG). + # + # Schema source: TBXcoreStructV03.rng `<define name="ref">`; + # data category: Basic.tbxmd. class Ref < Lutaml::Model::Serializable - attribute :id, :string - attribute :lang, Lutaml::Xml::W3c::XmlLangType - attribute :target, :string - attribute :datatype, :string - attribute :type, :string - attribute :content, :string, collection: true + include Tbx::DataElement + + TYPES = Modules::Basic::REF_TYPES.freeze xml do root "ref" diff --git a/lib/tbx/ref_object.rb b/lib/tbx/ref_object.rb index 5d7c15e..14805df 100644 --- a/lib/tbx/ref_object.rb +++ b/lib/tbx/ref_object.rb @@ -1,6 +1,12 @@ # frozen_string_literal: true module Tbx + # A reference object `<refObject>` defining a picklist or value set. + # + # Contains `itemSet`, `itemGrp`, or `item` children that enumerate the + # permitted values for a data category's picklist. + # + # Schema source: TBXcoreStructV03.rng `<define name="refObject">` class RefObject < Lutaml::Model::Serializable attribute :id, :string attribute :item_set, ::Tbx::ItemSet, collection: true diff --git a/lib/tbx/ref_object_sec.rb b/lib/tbx/ref_object_sec.rb index cedc550..4d57215 100644 --- a/lib/tbx/ref_object_sec.rb +++ b/lib/tbx/ref_object_sec.rb @@ -1,6 +1,12 @@ # frozen_string_literal: true module Tbx + # Reference object section `<refObjectSec>` in back matter. + # + # Contains reference objects that define picklists and value sets used + # by data category elements throughout the termbase. + # + # Schema source: TBXcoreStructV03.rng `<define name="refObjectSec">` class RefObjectSec < Lutaml::Model::Serializable attribute :id, :string attribute :type, :string diff --git a/lib/tbx/revision_desc.rb b/lib/tbx/revision_desc.rb index bbd041a..9ca37ab 100644 --- a/lib/tbx/revision_desc.rb +++ b/lib/tbx/revision_desc.rb @@ -1,6 +1,9 @@ # frozen_string_literal: true module Tbx + # Revision description `<revisionDesc>`. + # + # Schema source: TBXcoreStructV03.rng `<define name="revisionDesc">` class RevisionDesc < Lutaml::Model::Serializable attribute :id, :string attribute :lang, Lutaml::Xml::W3c::XmlLangType diff --git a/lib/tbx/sc.rb b/lib/tbx/sc.rb index 7ea1748..46bea27 100644 --- a/lib/tbx/sc.rb +++ b/lib/tbx/sc.rb @@ -1,12 +1,18 @@ # frozen_string_literal: true module Tbx + # XLIFF inline start-code marker `<sc>`. + # + # Used for representing inline formatting codes from source formats. + # The `id` is required and is referenced by a corresponding `<ec>` + # element's `startRef`. + # + # Attributes per core RNG: `id` (required, type ID), `isolated` (optional, + # yes/no). + # Schema source: TBXcoreStructV03.rng `<define name="sc">` class Sc < Lutaml::Model::Serializable attribute :id, :string attribute :isolated, :string - attribute :type, :string - attribute :subtype, :string - attribute :target, :string xml do root "sc" @@ -14,9 +20,6 @@ class Sc < Lutaml::Model::Serializable map_attribute "id", to: :id map_attribute "isolated", to: :isolated - map_attribute "type", to: :type - map_attribute "subtype", to: :subtype - map_attribute "target", to: :target end end end diff --git a/lib/tbx/source_desc.rb b/lib/tbx/source_desc.rb index 8ce6618..7340861 100644 --- a/lib/tbx/source_desc.rb +++ b/lib/tbx/source_desc.rb @@ -1,6 +1,9 @@ # frozen_string_literal: true module Tbx + # Source description `<sourceDesc>`. + # + # Schema source: TBXcoreStructV03.rng `<define name="sourceDesc">` class SourceDesc < Lutaml::Model::Serializable attribute :id, :string attribute :lang, Lutaml::Xml::W3c::XmlLangType diff --git a/lib/tbx/tbx_header.rb b/lib/tbx/tbx_header.rb index c9178b1..e66d446 100644 --- a/lib/tbx/tbx_header.rb +++ b/lib/tbx/tbx_header.rb @@ -1,6 +1,13 @@ # frozen_string_literal: true module Tbx + # Document header `<tbxHeader>`. + # + # Contains file description, encoding information, and revision history. + # Children: `fileDesc` (required), `encodingDesc` (optional), + # `revisionDesc` (optional). + # + # Schema source: TBXcoreStructV03.rng `<define name="tbxHeader">` class TbxHeader < Lutaml::Model::Serializable attribute :id, :string attribute :file_desc, ::Tbx::FileDesc diff --git a/lib/tbx/term.rb b/lib/tbx/term.rb index ec0b8ce..358b14f 100644 --- a/lib/tbx/term.rb +++ b/lib/tbx/term.rb @@ -1,6 +1,12 @@ # frozen_string_literal: true module Tbx + # The term designation element `<term>`. + # + # Contains the actual term text. Content is limited to plain text and + # `<hi>` inline highlighting elements per the `entity.basicText` pattern. + # + # Schema source: TBXcoreStructV03.rng `<define name="term">` class Term < Lutaml::Model::Serializable attribute :id, :string attribute :content, :string, collection: true diff --git a/lib/tbx/term_comp.rb b/lib/tbx/term_comp.rb new file mode 100644 index 0000000..6db002d --- /dev/null +++ b/lib/tbx/term_comp.rb @@ -0,0 +1,26 @@ +# frozen_string_literal: true + +module Tbx + # A single component of a decomposed term `<termComp>`. + # + # Used for representing hyphenation, syllabification, morphological + # elements, lemmata, or other logically significant portions of a term. + # Content is plain text only. + # + # Schema source: TermComp-namespace.rng `<define name="termComp">` + class TermComp < Lutaml::Model::Serializable + attribute :id, :string + attribute :lang, Lutaml::Xml::W3c::XmlLangType + attribute :content, :string, collection: true + + xml do + root "termComp" + mixed_content + namespace ::Tbx::Namespace + + map_attribute "id", to: :id + w3c_attributes :lang + map_content to: :content + end + end +end diff --git a/lib/tbx/term_comp_grp.rb b/lib/tbx/term_comp_grp.rb new file mode 100644 index 0000000..70577d8 --- /dev/null +++ b/lib/tbx/term_comp_grp.rb @@ -0,0 +1,24 @@ +# frozen_string_literal: true + +module Tbx + # Term component group `<termCompGrp>`. + # + # Groups a `<termComp>` with associated `<note>` elements. + # + # Schema source: TermComp-namespace.rng `<define name="termCompGrp">` + class TermCompGrp < Lutaml::Model::Serializable + attribute :id, :string + attribute :term_comp, ::Tbx::TermComp + attribute :note, ::Tbx::Note, collection: true + + xml do + root "termCompGrp" + mixed_content + namespace ::Tbx::Namespace + + map_attribute "id", to: :id + map_element "termComp", to: :term_comp + map_element "note", to: :note + end + end +end diff --git a/lib/tbx/term_comp_sec.rb b/lib/tbx/term_comp_sec.rb new file mode 100644 index 0000000..af25b64 --- /dev/null +++ b/lib/tbx/term_comp_sec.rb @@ -0,0 +1,45 @@ +# frozen_string_literal: true + +module Tbx + # Term component section `<termCompSec>`. + # + # Section containing decomposed term components. The `type` attribute + # indicates the decomposition method. + # + # Permitted `type` values (from TermComp-namespace.rng): + # + # * `hyphenation` — parts of a term as it would be hyphenated + # * `lemma` — base form (dictionary entry form) + # * `morphologicalElement` — individual morphemes comprising the term + # * `syllabification` — individual syllables comprising the term + # * `termElement` — any other logically significant portion + # + # Schema source: TermComp-namespace.rng `<define name="termCompSec">` + class TermCompSec < Lutaml::Model::Serializable + TYPES = { + hyphenation: "hyphenation", + lemma: "lemma", + morphological_element: "morphologicalElement", + syllabification: "syllabification", + term_element: "termElement", + }.freeze + + attribute :id, :string + attribute :type, :string + attribute :note, ::Tbx::Note, collection: true + attribute :term_comp, ::Tbx::TermComp, collection: true + attribute :term_comp_grp, ::Tbx::TermCompGrp, collection: true + + xml do + root "termCompSec" + mixed_content + namespace ::Tbx::Namespace + + map_attribute "id", to: :id + map_attribute "type", to: :type + map_element "note", to: :note + map_element "termComp", to: :term_comp + map_element "termCompGrp", to: :term_comp_grp + end + end +end diff --git a/lib/tbx/term_note.rb b/lib/tbx/term_note.rb index 8d27091..f3d5c97 100644 --- a/lib/tbx/term_note.rb +++ b/lib/tbx/term_note.rb @@ -1,18 +1,51 @@ # frozen_string_literal: true module Tbx + # Term-level data category element `<termNote>`. + # + # Carries grammatical, administrative, and usage information about a term. + # Only allowed as a child of `<termSec>` or `<termNoteGrp>`. + # + # Permitted `type` values (composed from all modules): + # + # * Min module: `administrativeStatus` (picklist: admittedTerm-admn-sts, + # deprecatedTerm-admn-sts, supersededTerm-admn-sts, preferredTerm-admn-sts), + # `partOfSpeech` (picklist: adjective, noun, other, verb, adverb) + # * Basic module: `geographicalUsage` (string), `grammaticalGender` + # (picklist: masculine, feminine, neuter, other), `termLocation` + # (picklist: 18 UI element types), `termType` (picklist: fullForm, + # acronym, abbreviation, shortForm, variant, phrase) + # * Linguist module: `grammaticalNumber` (picklist: singular, plural, dual, + # mass, otherNumber), `register` (picklist: colloquialRegister, + # neutralRegister, technicalRegister, in-houseRegister, + # bench-levelRegister, slangRegister, vulgarRegister), + # `transferComment` (string) + # + # Content model: `entity.noteText` (mixed text + inline elements hi, ec, + # foreign, ph, sc). + # + # @see TYPES + # + # Schema source: TBXcoreStructV03.rng `<define name="termNote">`; + # data categories: Min.tbxmd, Basic.tbxmd, Linguist.tbxmd; + # permitted types validated by DCA Schematron (e.g. TBX-Basic_DCA.sch). class TermNote < Lutaml::Model::Serializable - attribute :id, :string - attribute :lang, Lutaml::Xml::W3c::XmlLangType - attribute :target, :string - attribute :datatype, :string - attribute :type, :string - attribute :content, :string, collection: true - attribute :hi, ::Tbx::Hi, collection: true - attribute :ec, ::Tbx::Ec, collection: true - attribute :foreign, ::Tbx::Foreign, collection: true - attribute :ph, ::Tbx::Ph, collection: true - attribute :sc, ::Tbx::Sc, collection: true + include Tbx::DataElement + include Tbx::DataElement::InlineContent + + # Permitted termNote/@type values per TBX-Basic DCA Schematron + # (ISO 30042:2019, TBX-Basic dialect, DCA style). + # + # Source: reference-docs/schemas/TBX-Basic_DCA.sch line 54-56 + # "Permitted type value(s): administrativeStatus, partOfSpeech, + # geographicalUsage, grammaticalGender, termLocation, termType" + TYPES = Modules::Min::TERM_NOTE_TYPES + .merge(Modules::Basic::TERM_NOTE_TYPES) + .merge(Modules::Linguist::TERM_NOTE_TYPES).freeze + + VALUES = Modules::Min::TERM_NOTE_VALUES + .merge(Modules::Basic::TERM_NOTE_VALUES) + .merge(Modules::Linguist::TERM_NOTE_VALUES).freeze xml do root "termNote" diff --git a/lib/tbx/term_note_grp.rb b/lib/tbx/term_note_grp.rb index 91cffb3..b71a185 100644 --- a/lib/tbx/term_note_grp.rb +++ b/lib/tbx/term_note_grp.rb @@ -1,6 +1,13 @@ # frozen_string_literal: true module Tbx + # Groups a `<termNote>` with its associated administrative data and + # references. + # + # Children: `termNote` (required), then entity.noteLinkInfo (admin, + # adminGrp, note, ref, transacGrp, xref). + # + # Schema source: TBXcoreStructV03.rng `<define name="termNoteGrp">` class TermNoteGrp < Lutaml::Model::Serializable attribute :id, :string attribute :term_note, ::Tbx::TermNote diff --git a/lib/tbx/term_sec.rb b/lib/tbx/term_sec.rb index 8d98ea0..437a2eb 100644 --- a/lib/tbx/term_sec.rb +++ b/lib/tbx/term_sec.rb @@ -1,6 +1,14 @@ # frozen_string_literal: true module Tbx + # Term section `<termSec>`. + # + # Contains a single term designation and its associated term-level notes + # and administrative data. Children: `term` (required), then + # termNote/termNoteGrp, then auxInfo elements (admin, adminGrp, descrip, + # descripGrp, note, ref, transacGrp, xref). + # + # Schema source: TBXcoreStructV03.rng `<define name="termSec">` class TermSec < Lutaml::Model::Serializable attribute :id, :string attribute :term, ::Tbx::Term diff --git a/lib/tbx/text_element.rb b/lib/tbx/text_element.rb index 6a67f5a..ea8dae1 100644 --- a/lib/tbx/text_element.rb +++ b/lib/tbx/text_element.rb @@ -1,6 +1,11 @@ # frozen_string_literal: true module Tbx + # Wrapper element `<text>` for the termbase body and back matter. + # + # Children: `body` (optional), `back` (optional). + # + # Schema source: TBXcoreStructV03.rng `<define name="text">` class TextElement < Lutaml::Model::Serializable attribute :id, :string attribute :body, ::Tbx::Body diff --git a/lib/tbx/title.rb b/lib/tbx/title.rb index d4a1ec6..3c0c4a2 100644 --- a/lib/tbx/title.rb +++ b/lib/tbx/title.rb @@ -1,6 +1,12 @@ # frozen_string_literal: true module Tbx + # Title element `<title>`. + # + # Used within `<titleStmt>` to specify the title of the TBX file. + # Content is plain text only. + # + # Schema source: TBXcoreStructV03.rng `<define name="title">` class Title < Lutaml::Model::Serializable attribute :id, :string attribute :lang, Lutaml::Xml::W3c::XmlLangType diff --git a/lib/tbx/title_stmt.rb b/lib/tbx/title_stmt.rb index d1d0665..af82ac2 100644 --- a/lib/tbx/title_stmt.rb +++ b/lib/tbx/title_stmt.rb @@ -1,6 +1,9 @@ # frozen_string_literal: true module Tbx + # Title statement `<titleStmt>`. + # + # Schema source: TBXcoreStructV03.rng `<define name="titleStmt">` class TitleStmt < Lutaml::Model::Serializable attribute :id, :string attribute :lang, Lutaml::Xml::W3c::XmlLangType diff --git a/lib/tbx/transac.rb b/lib/tbx/transac.rb index 974fe0c..266d28b 100644 --- a/lib/tbx/transac.rb +++ b/lib/tbx/transac.rb @@ -1,13 +1,24 @@ # frozen_string_literal: true module Tbx + # Transaction element `<transac>`. + # + # Records an action performed on a terminological entry. The content + # indicates the type of transaction (origination or modification). + # + # Permitted `type` values: + # + # * Basic module: `transactionType` (picklist: `origination`, `modification`) + # + # Content is plain text only (no inline elements per the core RNG). + # + # Schema source: TBXcoreStructV03.rng `<define name="transac">`; + # data category: Basic.tbxmd. class Transac < Lutaml::Model::Serializable - attribute :id, :string - attribute :lang, Lutaml::Xml::W3c::XmlLangType - attribute :target, :string - attribute :datatype, :string - attribute :type, :string - attribute :content, :string, collection: true + include Tbx::DataElement + + TYPES = Modules::Basic::TRANSAC_TYPES.freeze + VALUES = Modules::Basic::TRANSAC_VALUES.freeze xml do root "transac" diff --git a/lib/tbx/transac_grp.rb b/lib/tbx/transac_grp.rb index 9abdcbd..2d5a315 100644 --- a/lib/tbx/transac_grp.rb +++ b/lib/tbx/transac_grp.rb @@ -1,6 +1,12 @@ # frozen_string_literal: true module Tbx + # Groups a `<transac>` transaction element with its date and + # responsibility information. + # + # Children: `transac` (required), then date, note, ref, transacNote, xref. + # + # Schema source: TBXcoreStructV03.rng `<define name="transacGrp">` class TransacGrp < Lutaml::Model::Serializable attribute :id, :string attribute :transac, ::Tbx::Transac diff --git a/lib/tbx/transac_note.rb b/lib/tbx/transac_note.rb index 9beefe6..0c55de8 100644 --- a/lib/tbx/transac_note.rb +++ b/lib/tbx/transac_note.rb @@ -1,13 +1,24 @@ # frozen_string_literal: true module Tbx + # Transaction note element `<transacNote>`. + # + # Provides additional information about a transaction, typically identifying + # the person or organization responsible. + # + # Permitted `type` values: + # + # * Basic module: `responsibility` — person/org responsible for the + # transaction (DC-451) + # + # Content is plain text only (no inline elements per the core RNG). + # + # Schema source: TBXcoreStructV03.rng `<define name="transacNote">`; + # data category: Basic.tbxmd. class TransacNote < Lutaml::Model::Serializable - attribute :id, :string - attribute :lang, Lutaml::Xml::W3c::XmlLangType - attribute :target, :string - attribute :datatype, :string - attribute :type, :string - attribute :content, :string, collection: true + include Tbx::DataElement + + TYPES = Modules::Basic::TRANSAC_NOTE_TYPES.freeze xml do root "transacNote" diff --git a/lib/tbx/xref.rb b/lib/tbx/xref.rb index 6c8c68c..1624653 100644 --- a/lib/tbx/xref.rb +++ b/lib/tbx/xref.rb @@ -1,7 +1,23 @@ # frozen_string_literal: true module Tbx + # External cross-reference element `<xref>`. + # + # The `target` attribute holds a URI (http/https) pointing to an external + # resource. Unlike `Ref`, which uses IDREF for internal references, Xref + # uses anyURI for external resources. + # + # Permitted `type` values: + # + # * Min module: `externalCrossReference` — reference to an external resource + # * Basic module: `externalCrossReference` — external reference (DC-226), + # `xGraphic` — graphic image associated with the concept (DC-2920) + # + # Schema source: TBXcoreStructV03.rng `<define name="xref">`; + # data categories: Basic.tbxmd. class Xref < Lutaml::Model::Serializable + TYPES = Modules::Min::XREF_TYPES + .merge(Modules::Basic::XREF_TYPES).freeze attribute :id, :string attribute :target, :string attribute :type, :string diff --git a/reference-docs/README.adoc b/reference-docs/README.adoc new file mode 100644 index 0000000..9c1e260 --- /dev/null +++ b/reference-docs/README.adoc @@ -0,0 +1,109 @@ += Reference Documentation + +This directory contains official TBX schema, dialect, and module reference +files from https://ltac-global.org[LTAC Global] (LTAC-Global on GitHub). + +== Source repositories + +All files below are sourced from the +https://github.com/LTAC-Global[LTAC-Global GitHub organization] and are +used under their respective licenses for reference purposes. + +=== Dialects + +Dialects define a specific profile of TBX with Schematron constraints, +RELAX NG schemas, and example files. + +|=== +| Directory | Source repository | Description + +| `schemas/TBX-Basic_dialect_v1/` +| https://github.com/LTAC-Global/TBX-Basic_dialect[TBX-Basic_dialect] +| TBX-Basic dialect (DCA + DCT schemas, example files, bundled modules) + +| `schemas/TBX-Min_dialect/` +| https://github.com/LTAC-Global/TBX-Min_dialect[TBX-Min_dialect] +| TBX-Min dialect (DCA + DCT Schematron, NVDL) + +| `schemas/TBX-Core_dialect/` +| https://github.com/LTAC-Global/TBX-Core_dialect[TBX-Core_dialect] +| TBX-Core dialect (integrated RNG, Schematron, example) + +| `schemas/TBX-Linguist_dialect/` +| https://github.com/LTAC-Global/TBX-Linguist_dialect[TBX-Linguist_dialect] +| TBX-Linguist dialect (DCA + DCT Schematron, integrated RNG, examples) +|=== + +=== Modules + +Modules define data categories and structural rules for a specific level +of terminological detail. + +|=== +| Directory | Source repository | Key files + +| `schemas/TBX-Basic_dialect_v1/Modules/TBX_min_module/` +| https://github.com/LTAC-Global/TBX_min_module[TBX_min_module] +| `Min.rng`, `Min.sch`, `Min.tbxmd` + +| `schemas/TBX-Basic_dialect_v1/Modules/TBX_basic_module/` +| https://github.com/LTAC-Global/TBX_basic_module[TBX_basic_module] +| `Basic.rng`, `Basic.sch`, `Basic.tbxmd` + +| `schemas/TBX_linguist_module/` +| https://github.com/LTAC-Global/TBX_linguist_module[TBX_linguist_module] +| `Linguist.rng`, `Linguist.sch`, `Linguist.tbxmd` + +| `schemas/TBX_termComp_module/` +| https://github.com/LTAC-Global/TBX_termComp_module[TBX_termComp_module] +| `TermComp-namespace.rng` +|=== + +=== Core schema + +|=== +| File | Source repository | Description + +| `schemas/TBXcoreStructV03.rng` +| https://github.com/LTAC-Global/TBX_core_module[TBX_core_module] +| TBX core structural RELAX NG schema + +| `schemas/TBX_core.xsd` +| https://github.com/LTAC-Global/TBX_core_module[TBX_core_module] +| TBX core XML Schema (XSD) +|=== + +=== Module description format + +|=== +| Directory | Source repository | Key files + +| `schemas/TBX_module_description_xml/` +| https://github.com/LTAC-Global/TBX_module_description_xml[TBX_module_description_xml] +| `tbxmd.rng` -- RELAX NG schema for `.tbxmd` module definition files +|=== + +=== Implementation guide + +|=== +| Directory | Source repository | Key files + +| `schemas/TBX-Basic_ImplementationGuide/` +| https://github.com/LTAC-Global/TBX-Basic_ImplementationGuide[TBX-Basic_ImplementationGuide] +| `TBX-Basic_ImplementationGuide.pdf` +|=== + +== TBX module hierarchy + +The TBX standard (ISO 30042:2019) defines a modular architecture: + +.... +TBX-Core structural foundation (element definitions) + +-- TBX-Min minimal data categories for basic terminology + +-- TBX-Basic standard data categories for general terminology + +-- TBX-Linguist extended data categories for linguistic detail + +-- TBX-TermComp term composition and decomposition +.... + +Each dialect (TBX-Min, TBX-Basic, etc.) combines the core structure with +one or more modules and adds dialect-specific Schematron constraints. diff --git a/reference-docs/schemas/Basic_Module_Definition.pdf b/reference-docs/schemas/Basic_Module_Definition.pdf new file mode 100644 index 0000000..7b2b4b5 Binary files /dev/null and b/reference-docs/schemas/Basic_Module_Definition.pdf differ diff --git a/reference-docs/schemas/Min_Module_Definition.pdf b/reference-docs/schemas/Min_Module_Definition.pdf new file mode 100644 index 0000000..730f649 Binary files /dev/null and b/reference-docs/schemas/Min_Module_Definition.pdf differ diff --git a/reference-docs/schemas/TBX-Basic_ImplementationGuide/TBX-Basic_ImplementationGuide.pdf b/reference-docs/schemas/TBX-Basic_ImplementationGuide/TBX-Basic_ImplementationGuide.pdf new file mode 100644 index 0000000..e9b5933 Binary files /dev/null and b/reference-docs/schemas/TBX-Basic_ImplementationGuide/TBX-Basic_ImplementationGuide.pdf differ diff --git a/reference-docs/schemas/TBX-Core_dialect/Schemas/Example_Astronomy_DCA_VALID.tbx b/reference-docs/schemas/TBX-Core_dialect/Schemas/Example_Astronomy_DCA_VALID.tbx new file mode 100644 index 0000000..50fe4c7 --- /dev/null +++ b/reference-docs/schemas/TBX-Core_dialect/Schemas/Example_Astronomy_DCA_VALID.tbx @@ -0,0 +1,710 @@ +<?xml version="1.0" encoding="utf-8"?> +<?xml-model href="https://raw.githubusercontent.com/LTAC-Global/TBX-Core_dialect/master/Schemas/TBXcoreStructV03_TBX-Core_integrated.rng" type="application/xml" schematypens="http://relaxng.org/ns/structure/1.0"?> +<?xml-model href="https://raw.githubusercontent.com/LTAC-Global/TBX-Core_dialect/master/Schemas/TBX-Core.sch" type="application/xml" schematypens="http://purl.oclc.org/dsdl/schematron"?> +<tbx type="TBX-Core" style="dca" xml:lang="en" xmlns="urn:iso:std:iso:30042:ed-2"> + <tbxHeader> + <fileDesc> + <sourceDesc> + <p>TBX file, created via MultiTerm Export</p> + </sourceDesc> + </fileDesc> + </tbxHeader> + <text> + <body> + <conceptEntry id="c1"> + <langSec xml:lang="en"> + <termSec> + <term>open cluster</term> + </termSec> + <termSec> + <term>galactic cluster</term> + <note>Another name for an open star cluster. They are often termed Galactic + Clusters because they are found mainly in the plane of our galaxy. If + you were to view our galaxy from afar, you would find that all the + open/galactic clusters lie within the spiral arms of the galaxy.</note> + <note>N-Source: + http://www.delscope.demon.co.uk/astronomy/glossary.htm#G</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo abierto</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c2"> + <langSec xml:lang="en"> + <termSec> + <term>circumstellar accretion disk</term> + </termSec> + <termSec> + <term>accretion disc</term> + </termSec> + <termSec> + <term>circumstellar disk</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>disco de acreción</term> + </termSec> + <termSec> + <term>disco de acrecimiento</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c3"> + <langSec xml:lang="en"> + <termSec> + <term>black hole</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>agujero negro</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c4"> + <langSec xml:lang="en"> + <termSec> + <term>gamma-ray burst</term> + </termSec> + <termSec> + <term>GRB</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>explosión de rayos gamma</term> + </termSec> + <termSec> + <term>brote de rayos gamma</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c5"> + <langSec xml:lang="en"> + <termSec> + <term>globular cluster</term> + <note>Related Term: star cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo globular</term> + <note>Related Term: cúmulo estelar</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c6"> + <langSec xml:lang="en"> + <termSec> + <term>main-sequence</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>de secuencia principal</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c7"> + <langSec xml:lang="en"> + <termSec> + <term>protostar</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>protoestrella</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c8"> + <langSec xml:lang="en"> + <termSec> + <term>star cluster</term> + <note>Related Term: globular cluster</note> + <note>Related Term: open cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo estelar</term> + </termSec> + <termSec> + <term>cúmulo de estrellas</term> + <note>Related Term: cúmulo globular</note> + <note>Related Term: cúmulo abierto</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c9"> + <langSec xml:lang="en"> + <termSec> + <term>Galaxy</term> + </termSec> + <termSec> + <term>Milky Way Galaxy</term> + </termSec> + <termSec> + <term>Milky Way</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>Galaxia</term> + </termSec> + <termSec> + <term>Vía Láctea</term> + </termSec> + <termSec> + <term>galaxia Vía Láctea</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c10"> + <langSec xml:lang="en"> + <termSec> + <term>star</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c11"> + <langSec xml:lang="en"> + <termSec> + <term>UV radiation</term> + </termSec> + <termSec> + <term>ultraviolet radiation</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>radiación UV</term> + </termSec> + <termSec> + <term>radiación ultravioleta</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c12"> + <langSec xml:lang="en"> + <termSec> + <term>magnetic field</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>campo magnético</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c13"> + <langSec xml:lang="en"> + <termSec> + <term>blue straggler</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella rezagada azul</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c14"> + <langSec xml:lang="en"> + <termSec> + <term>gravitational collapse</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>colapso gravitacional</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c15"> + <langSec xml:lang="en"> + <termSec> + <term>binary star</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella binaria</term> + </termSec> + <termSec> + <term>estrella doble</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c16"> + <note>This figure compares the IMFs by ploting mass fraction per dex versus mass, + i.e., normalized so that the integral under each curve is unity. They are + assumed to be valid from 0.1 to 120 solar masses.</note> + <note>N-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <langSec xml:lang="en"> + <termSec> + <term>initial mass function</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>función inicial de masa</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c17"> + <langSec xml:lang="zu"> + <termSec> + <term>Bally2005</term> + <note>Author[s]: Bally, John and Hans Zinnecker</note> + <note>Journal Title: The Astronomical Journal</note> + <note>Article Title: The Birth of High-Mass Stars: Accertion and/or + Mergers?</note> + <note>Volume: 129</note> + <note>Publication Place: U.S.A.</note> + <note>Publisher: The American Astronomical Society</note> + <note>Publication Year: May 2005</note> + <note>Page(s): 2281-2293</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c18"> + <langSec xml:lang="zu"> + <termSec> + <term>Cambridge2007</term> + <note>Author[s]: Mitton, Jaqueline</note> + <note>Book Title: Cambridge Illustrated Dictionary of Astronomy</note> + <note>Publication Place: New York</note> + <note>Publisher: Cambridge University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c19"> + <langSec xml:lang="zu"> + <termSec> + <term>Merriam-Webster2002</term> + <note>Book Title: Webster's Third New International Dictionary</note> + <note>Editor[s]: Gove, Philip Babcock</note> + <note>Volume: Third Edition</note> + <note>Publication Place: Springfield, Massachusetts</note> + <note>Publisher: Merriam-Webster INC.</note> + <note>Publication Year: 2002</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c20"> + <langSec xml:lang="zu"> + <termSec> + <term>Oxford2007</term> + <note>Book Title: Oxford Dictionary of Astronomy</note> + <note>Editor[s]: Ridpath, Ian</note> + <note>Volume: Second Edition</note> + <note>Publication Place: New York</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c21"> + <langSec xml:lang="en"> + <termSec> + <term>supernova</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>supernova</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c22"> + <langSec xml:lang="zu"> + <termSec> + <term>Moore2003</term> + <note>Author[s]: Moore, Patrick</note> + <note>Book Title: Philip's Atlas of the Universe</note> + <note>Publication Place: Heron Quays, London</note> + <note>Publisher: Philip's</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c23"> + <langSec xml:lang="en"> + <termSec> + <term>red giant</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>gigante roja</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c24"> + <langSec xml:lang="en"> + <termSec> + <term>red dwarf</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana roja</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c25"> + <langSec xml:lang="en"> + <termSec> + <term>spectral type</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>tipo espectral</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c26"> + <langSec xml:lang="en"> + <note>This is the end-result of all but the most massive of stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>white dwarf</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana blanca</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c27"> + <langSec xml:lang="en"> + <note>As mass is gradually lost, the core of the star becomes more exposed, + ultimately becoming a white dwarf. Also, planetary nebulae have nothing to + do with planets, and are not true nebulae.</note> + <note>N-Source: Based on Oxford2007 and Moore2003, 186</note> + <termSec> + <term>planetary nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa planetaria</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c28"> + <langSec xml:lang="en"> + <note>Ultraviolet radiation, gas cloud collisions, and synchrotron radiation can + all cause the emission nebula to shine.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>emission nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa de emisión</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c29"> + <langSec xml:lang="en"> + <note>The term was originally applied to any object with a fuzzy telescopic + appearance, but with the advent of larger instruments many 'nebulae' were + found to consist of faint stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>nebula</term> + <note>Grammatical Number: singular</note> + </termSec> + <termSec> + <term>nebulae</term> + <note>Grammatical Number: plural</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c30"> + <langSec xml:lang="en"> + <termSec> + <term>dark nebula</term> + </termSec> + <termSec> + <term>absorbtion nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa oscura</term> + </termSec> + <termSec> + <term>nebulosa de absorción</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c31"> + <langSec xml:lang="en"> + <termSec> + <term>reflection nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa de reflexión</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c32"> + <langSec xml:lang="en"> + <termSec> + <term>neutron star</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella de neutrones</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c33"> + <langSec xml:lang="en"> + <note>For a star with no hydrogen content the limit is 1.44 solar masses, which + is thus the maximum possible for a white dwarf.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>Chandrasekhar limit</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>límite de Chandrasekhar</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c34"> + <langSec xml:lang="en"> + <note>Encountered on in neutron stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>neutron degeneracy</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración de neutrones</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c35"> + <langSec xml:lang="en"> + <termSec> + <term>Schwarzschild radius</term> + <note>Related Term: event horizon</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>radio de Schwarzschild</term> + <note>Related Term: horizonte de sucesos, horizonte de eventos</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c36"> + <langSec xml:lang="en"> + <termSec> + <term>event horizon</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>horizonte de sucesos</term> + </termSec> + <termSec> + <term>horizonte de eventos</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c37"> + <langSec xml:lang="en"> + <termSec> + <term>proton-proton chain reaction</term> + </termSec> + <termSec> + <term>PP chain</term> + </termSec> + <termSec> + <term>proton-proton reaction</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cadena protón-protón</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c38"> + <langSec xml:lang="en"> + <termSec> + <term>carbon-nitrogen cycle</term> + </termSec> + <termSec> + <term>CNO cycle</term> + </termSec> + <termSec> + <term>carbon-nitrogen-oxygen cycle</term> + </termSec> + <termSec> + <term>Bethe-Weizsäcker-cycle</term> + </termSec> + <termSec> + <term>carbon cycle</term> + <note>The carbon cycle can also refer to the biogeochemical cycle by which + carbon is exchanged among the biosphere, pedosphere, geosphere, + hydrosphere, and atmosphere of the Earth.</note> + <note>N-Source: http://en.wikipedia.org/wiki/Carbon_cycle</note> + </termSec> + <termSec> + <term>CN cycle</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>ciclo CNO</term> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno-oxígeno</term> + </termSec> + <termSec> + <term>ciclo del carbono</term> + <note>También este término puede referirse a la formación de las moléculas + de carbohidratos, lípidos, proteínas y ácidos nucleicos.</note> + <note>N-Source: http://es.wikipedia.org/wiki/Ciclo_del_carbono</note> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c39"> + <langSec xml:lang="en"> + <termSec> + <term>degeneracy</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c40"> + <langSec xml:lang="zu"> + <termSec> + <term>Oxford2003</term> + <note>Author[s]: Ridpath, Ian</note> + <note>Book Title: Astronomía</note> + <note>Publication Place: Spain</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c41"> + <langSec xml:lang="en"> + <note>Electron degeneracy supports white dwarf stars against further + collapse.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>electron degeneracy</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración de electrones</term> + </termSec> + <termSec> + <term>degeneración electrónica</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c42"> + <langSec xml:lang="en"> + <termSec> + <term>singularity</term> + <note>Related Term: black hole, event horizon, Schwarzschild radius</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>singularidad</term> + <note>Related Term: agujero negro, horizonte de sucesos, radio de + Schwarzschild</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c43"> + <note>In this graphic, the M with a subscript is the symbol for a solar mass.</note> + <note>N-Source: Jonathan Tomolonis</note> + <langSec xml:lang="en"> + <termSec> + <term>solar mass</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>masa solar</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c44"> + <langSec xml:lang="en"> + <termSec> + <term>triple-alpha process</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>proceso triple-alfa</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c45"> + <langSec xml:lang="en"> + <termSec> + <term>black dwarf</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana negra</term> + </termSec> + </langSec> + </conceptEntry> + </body> + <back> + <refObjectSec type="respPerson"> + <refObject id="pe324as3-9615-4d41-a9c8-30c36bffe0e6"> + <item type="fn">Tommy Tomolonis</item> + </refObject> + </refObjectSec> + </back> + </text> +</tbx> diff --git a/reference-docs/schemas/TBX-Core_dialect/Schemas/TBX-Core.sch b/reference-docs/schemas/TBX-Core_dialect/Schemas/TBX-Core.sch new file mode 100644 index 0000000..ad69c47 --- /dev/null +++ b/reference-docs/schemas/TBX-Core_dialect/Schemas/TBX-Core.sch @@ -0,0 +1,47 @@ +<?xml version="1.0" encoding="UTF-8"?> +<schema xmlns="http://purl.oclc.org/dsdl/schematron" queryBinding="xslt2" + xmlns:sqf="http://www.schematron-quickfix.com/validator/process"> + <ns uri="urn:iso:std:iso:30042:ed-2" prefix="tbx" /> + + <pattern id="coreEnforecement"> + <rule context="tbx:termNote"> + <assert test="parent::tbx:termSec or parent::tbx:termNoteGrp/parent::tbx:termSec">Any termNote is only allowed at the termSec level.</assert> + </rule> + <rule context="tbx:*[@type]"> + <assert test="@type != ''">Data category must be declared. If no permitted data categories are listed in the grammar schema, blank values are also not allowed.</assert> + </rule> + <rule context="*[@target]"> + <assert test="matches(@target,'https?://.+') or @target = //*/@id">ID must be IDREF for internal references or URI following HTTP protocol for external references.</assert> + </rule> + </pattern> + + <pattern id="XLIFF.inlineConstraints"> + <rule context="tbx:sc[following-sibling::tbx:ec]"> + <assert test="@isolated='no' or not(@isolated)">@isolated must be 'no' if <sc/> or <ec/> has its corresponding <sc/>/<ec/> in the same note text and @startRef must be used for <ec></assert> + </rule> + <rule context="tbx:ec[preceding-sibling::tbx:sc]"> + <assert test="@isolated='no' or not(@isolated)">@isolated must be 'no' if <sc/> or <ec/> has its corresponding <sc/>/<ec/> in the same note text and @startRef must be used for <ec></assert> + <assert test="@startRef">@starRef is required for <ec> if it is in the same note text as its corresponding <sc></assert> + <!--<assert test="not(@dir)">@dir only permitted when @isolated is 'yes'.</assert>--><!--@dir IS NOT CURRENTLY USED IN TBX--> + </rule> + <rule context="tbx:sc[not(following-sibling::tbx:ec)]"> + <assert test="@isolated='yes' or not(@isolated)">@isolated must be 'yes' if <sc/> or <ec/> does not have its corresponding <sc/>/<sc/> in the same note text</assert> + </rule> + <rule context="tbx:ec[not(preceding-sibling::tbx:sc)]"> + <assert test="@isolated='yes' or not(@isolated)">@isolated must be 'yes' if <sc/> or <ec/> does not have its corresponding <sc/>/<sc/> in the same note text</assert> + <assert test="@id">@id is REQUIRED when @isolated is or should be 'yes'.</assert> + </rule> + <rule context="tbx:ec[@isolated='yes']"> + <assert test="@id != ''">ID is required if @isolated is 'yes'.</assert> + </rule> + </pattern> + + <pattern id="dialectEnforcement"> + <rule context="tbx:tbx"> + <assert test="attribute::type='TBX-Core'">The name of this dialect should be TBX-Core</assert> + </rule> + <rule context="*[not(namespace-uri() = 'urn:iso:std:iso:30042:ed-2')]"> + <assert test="false()">No elements from foreign namespaces are permitted in the TBX-Core dialect.</assert> + </rule> + </pattern> +</schema> \ No newline at end of file diff --git a/reference-docs/schemas/TBX-Core_dialect/Schemas/TBXcoreStructV03_TBX-Core_integrated.rng b/reference-docs/schemas/TBX-Core_dialect/Schemas/TBXcoreStructV03_TBX-Core_integrated.rng new file mode 100644 index 0000000..624dde2 --- /dev/null +++ b/reference-docs/schemas/TBX-Core_dialect/Schemas/TBXcoreStructV03_TBX-Core_integrated.rng @@ -0,0 +1,1171 @@ +<?xml version="1.0" encoding="utf-8"?> +<grammar xmlns="http://relaxng.org/ns/structure/1.0" + datatypeLibrary="http://www.w3.org/2001/XMLSchema-datatypes" ns="urn:iso:std:iso:30042:ed-2"> + <define name="entity.basicText"> + <zeroOrMore> + <choice> + <text/> + <ref name="hi"/> + </choice> + </zeroOrMore> + </define> + <define name="entity.noteText"> + <zeroOrMore> + <choice> + <text/> + <ref name="hi"/> + <ref name="foreign"/> + <ref name="sc"/> + <ref name="ec"/> + <ref name="ph"/> + </choice> + </zeroOrMore> + </define> + <define name="entity.auxInfo"> + <choice> + <zeroOrMore> + <choice> + <ref name="descrip"/> + <ref name="descripGrp"/> + <ref name="admin"/> + <ref name="adminGrp"/> + <ref name="transacGrp"/> + <ref name="note"/> + <ref name="ref"/> + <ref name="xref"/> + </choice> + </zeroOrMore> + <zeroOrMore> + <choice> + <ref name="note"/> + <ref name="adminGrp"/> + <ref name="descripGrp"/> + <ref name="transacGrp"/> + <ref name="DCTnamespaceElements"/> + </choice> + </zeroOrMore> + </choice> + </define> + <define name="entity.noteLinkInfo"> + <choice> + <zeroOrMore> + <choice> + <ref name="admin"/> + <ref name="adminGrp"/> + <ref name="transacGrp"/> + <ref name="note"/> + <ref name="ref"/> + <ref name="xref"/> + </choice> + </zeroOrMore> + <zeroOrMore> + <choice> + <ref name="adminGrp"/> + <ref name="transacGrp"/> + <ref name="note"/> + <ref name="DCTnamespaceElements"/> + </choice> + </zeroOrMore> + </choice> + </define> + <define name="idlang.attributes"> + <ref name="id.attributes"/> + <ref name="lang.attributes"/> + </define> + <define name="idtype.attributes"> + <ref name="id.attributes"/> + <ref name="idtype.attribute.type"/> + </define> + <define name="idtype.attribute.type"> + <optional> + <attribute name="type"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the type of the meta data-category.</a:documentation> + <text/> + </attribute> + </optional> + </define> + <define name="id.attributes"> + <optional> + <ref name="id.attribute.id"/> + </optional> + </define> + <define name="id.attribute.id"> + <attribute name="id"> + <data type="ID"/> + </attribute> + </define> + <define name="target-IDREF.attributes"> + <ref name="target-IDREF.attribute.target"/> + </define> + <define name="target-IDREF.attribute.target"> + <optional> + <attribute name="target"> + + <data type="IDREF"/> + </attribute> + </optional> + </define> + <define name="lang.attributes"> + <ref name="lang.attribute.xmllang"/> + </define> + <define name="lang.attribute.xmllang"> + <optional> + <attribute name="xml:lang"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the language of the element content. The allowed values are found in IETF RFC 4646 or + its successor. This attribute is optional for elements that use this attribute class. + For a description, see the information at the tbx element.</a:documentation> + <data type="language"/> + </attribute> + </optional> + </define> + <define name="IDLangTgtDtyp.attributes"> + <ref name="lang.attributes"/> + <ref name="id.attributes"/> + <ref name="target-IDREF.attributes"/> + <ref name="IDLangTgtDtyp.attribute.datatype"/> + </define> + <define name="IDLangTgtDtyp.attribute.datatype"> + <optional> + <attribute name="datatype"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">The data + type of plainText, or what is known as PCDATA.</a:documentation> + <text/> + </attribute> + </optional> + </define> + <define name="dispEquivSubType.attributes"> + <optional> + <attribute name="disp"> + <text/> + </attribute> + <attribute name="equiv"> + <text/> + </attribute> + <choice> + <group> + <attribute name="subType"> + <data type="string"> + <param name="pattern">[^\s:]+:[^\s:]+</param> + </data> + </attribute> + <ref name="XLIFFinlineType.attribute"/> + </group> + <ref name="XLIFFinlineType.attribute"/> + </choice> + </optional> + </define> + <define name="XLIFFisolated.attribute"> + <optional> + <attribute name="isolated"> + <choice> + <value>yes</value> + <value>no</value> + </choice> + </attribute> + </optional> + </define> + <define name="XLIFFinlineType.attribute"> + <attribute name="type"> + <choice> + <value>fmt</value> + <value>ui</value> + <value>quote</value> + <value>link</value> + <value>image</value> + <value>other</value> + </choice> + </attribute> + </define> + <define name="hi"> + <element name="hi"> + + <ref name="hi.content"/> + <ref name="hi.localattributes"/> + </element> + </define> + <define name="hi.content"> + <text/> + </define> + <define name="hi.localattributes"> + <ref name="target-IDREF.attributes"/> + <ref name="lang.attributes"/> + <optional> + <attribute name="type"> + + <choice> + <value>entailedTerm</value> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0"> + (entailedTerm) A term, found in the content of a text element such as , that is + defined in another terminological entry in the same terminological + collection.</a:documentation> + <value>hotkey</value> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0"> + (hotkey) A key or a combination of keys on a computer keyboard that, when pressed + at one time, performs a task (such as starting an application) as an alternative + to using a mouse or other input device. Hotkeys are supported by many operating + systems and applications (the hotkey is indicated by an ampersand in the term and + by an underscore in the visual display). This type of hi element allows a hotkey + to be identified as such in a text field such as a context sentence. To identify a + hotkey for the head term of an entry, use the lionHotkey value of the type + attribute on a termNote.</a:documentation> + <value>italics</value> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0"> + (italics) Indicates that the content enclosed in the hi element must be rendered + in italics. </a:documentation> + <value>bold</value> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0"> + (bold) Indicates that the content enclosed in the hi element must be rendered in + boldface. </a:documentation> + <value>superscript</value> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0"> + (superscript) Indicates that the content enclosed in the hi element must be + rendered in superscript. </a:documentation> + <value>subscript</value> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0"> + (subscript) Indicates that the content enclosed in the hi element must be rendered + in subscript.</a:documentation> + <value>math</value> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0"> + (math) Indicates that the content enclosed in the hi element is mathematical in + nature.</a:documentation> + </choice> + </attribute> + </optional> + </define> + <define name="foreign"> + <element name="foreign"> + + <ref name="foreign.content"/> + <ref name="foreign.localattributes"/> + </element> + </define> + <define name="foreign.content"> + <ref name="entity.noteText"/> + </define> + <define name="foreign.localattributes"> + <ref name="idlang.attributes"/> + </define> + <define name="sc"> + <element name="sc"> + + <ref name="sc.content"/> + <ref name="sc.localattributes"/> + </element> + </define> + <define name="sc.content"> + <empty/> + </define> + <define name="sc.localattributes"> + <attribute name="id"> + <data type="ID"/> + </attribute> + <optional> + <ref name="dispEquivSubType.attributes"/> + <ref name="target-IDREF.attributes"/> + <ref name="XLIFFisolated.attribute"/> + </optional> + </define> + <define name="ec"> + <element name="ec"> + + <ref name="ec.content"/> + <ref name="ec.localattributes"/> + </element> + </define> + <define name="ec.content"> + <empty/> + </define> + <define name="ec.localattributes"> + <optional> + <attribute name="id"> + <data type="ID"/> + </attribute> + <attribute name="startRef"> + <data type="IDREF"/> + </attribute> + <ref name="dispEquivSubType.attributes"/> + <ref name="XLIFFisolated.attribute"/> + <ref name="target-IDREF.attributes"/> + </optional> + </define> + <define name="ph"> + <element name="ph"> + + <ref name="ph.content"/> + <ref name="ph.localattributes"/> + </element> + </define> + <define name="ph.content"> + <empty/> + </define> + <define name="ph.localattributes"> + <optional> + <attribute name="id"> + <data type="ID"/> + </attribute> + <ref name="dispEquivSubType.attributes"/> + </optional> + </define> + <define name="admin"> + <element name="admin"> + + <ref name="admin.content"/> + <ref name="admin.localattributes"/> + </element> + </define> + <define name="admin.content"> + <ref name="entity.noteText"/> + </define> + <define name="admin.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the data-category type of the admin element, such as originatingDatabase or + entrySource.</a:documentation> + + <ref name="admin.types"/> + + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="adminGrp"> + <element name="adminGrp"> + + <ref name="adminGrp.content"/> + <ref name="adminGrp.localattributes"/> + </element> + </define> + <define name="adminGrp.content"> + <choice> + <group> + <ref name="admin"/> + <zeroOrMore> + <choice> + <ref name="adminNote"/> + <ref name="note"/> + <ref name="ref"/> + <ref name="xref"/> + </choice> + </zeroOrMore> + </group> + <group> + <ref name="DCTnamespaceElements"/> + <zeroOrMore> + <choice> + <ref name="note"/> + <ref name="DCTnamespaceElements"/> + </choice> + </zeroOrMore> + </group> + </choice> + </define> + <define name="adminGrp.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="adminNote"> + <element name="adminNote"> + + <ref name="adminNote.content"/> + <ref name="adminNote.localattributes"/> + </element> + </define> + <define name="adminNote.content"> + <text/> + </define> + <define name="adminNote.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + + + <ref name="adminNote.types"/> + + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="date"> + <element name="date"> + + <ref name="date.content"/> + <ref name="date.localattributes"/> + </element> + </define> + <define name="date.content"> + <data type="date"/> + </define> + <define name="date.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="descrip"> + <element name="descrip"> + + <ref name="descrip.content"/> + <ref name="descrip.localattributes"/> + </element> + </define> + <define name="descrip.content"> + <ref name="entity.noteText"/> + </define> + <define name="descrip.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the data-category type of the descrip element, such as definition or + associated-concept.</a:documentation> + + <ref name="descrip.types"/> + + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="descripGrp"> + <element name="descripGrp"> + + <ref name="descripGrp.content"/> + <ref name="descripGrp.localattributes"/> + </element> + </define> + <define name="descripGrp.content"> + <choice> + <group> + <ref name="descrip"/> + <zeroOrMore> + <choice> + <ref name="descripNote"/> + <ref name="admin"/> + <ref name="adminGrp"/> + <ref name="transacGrp"/> + <ref name="note"/> + <ref name="ref"/> + <ref name="xref"/> + </choice> + </zeroOrMore> + </group> + <group> + <ref name="DCTnamespaceElements"/> + <zeroOrMore> + <choice> + <ref name="note"/> + <ref name="adminGrp"/> + <ref name="transacGrp"/> + <ref name="DCTnamespaceElements"/> + </choice> + </zeroOrMore> + </group> + </choice> + </define> + <define name="descripGrp.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="descripNote"> + <element name="descripNote"> + + <ref name="descripNote.content"/> + <ref name="descripNote.localattributes"/> + </element> + </define> + <define name="descripNote.content"> + <text/> + </define> + <define name="descripNote.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the data-category type of the descripNote element, such as + contextType.</a:documentation> + + <ref name="descripNote.types"/> + + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="langSec"> + <element name="langSec"> + + <ref name="langSec.content"/> + <ref name="langSec.localattributes"/> + </element> + </define> + <define name="langSec.content"> + <ref name="entity.auxInfo"/> + <oneOrMore> + <choice> + <ref name="termSec"/> + </choice> + </oneOrMore> + </define> + <define name="langSec.localattributes"> + <attribute name="xml:lang"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the language of the language section. This attribute is required for the langSec + element. See also the description on the tbx element.</a:documentation> + <text/> + </attribute> + </define> + <define name="note"> + <element name="note"> + + <ref name="note.content"/> + <ref name="note.localattributes"/> + </element> + </define> + <define name="note.content"> + <ref name="entity.noteText"/> + </define> + <define name="note.localattributes"> + <ref name="idlang.attributes"/> + </define> + <define name="ref"> + <element name="ref"> + + <ref name="ref.content"/> + <ref name="ref.localattributes"/> + </element> + </define> + <define name="ref.content"> + <text/> + </define> + <define name="ref.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + + + <ref name="ref.types"/> + + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="term"> + <element name="term"> + <ref name="term.content"/> + <ref name="term.localattributes"/> + </element> + </define> + <define name="term.content"> + <ref name="entity.basicText"/> + </define> + <define name="term.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="conceptEntry"> + <element name="conceptEntry"> + + <ref name="conceptEntry.content"/> + <ref name="conceptEntry.localattributes"/> + </element> + </define> + <define name="conceptEntry.content"> + <ref name="entity.auxInfo"/> + <oneOrMore> + <ref name="langSec"/> + </oneOrMore> + </define> + <define name="conceptEntry.localattributes"> + <ref name="id.attribute.id"/> + </define> + <define name="termNote"> + <element name="termNote"> + <ref name="termNote.content"/> + <ref name="termNote.localattributes"/> + </element> + </define> + <define name="termNote.content"> + <ref name="entity.noteText"/> + </define> + <define name="termNote.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the data-category type of the termNote, such as partOfSpeech or + termType.</a:documentation> + <ref name="termNote.types"/> + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="termNoteGrp"> + <element name="termNoteGrp"> + <ref name="termNoteGrp.content"/> + <ref name="termNoteGrp.localattributes"/> + </element> + </define> + <define name="termNoteGrp.content"> + <choice> + <ref name="termNote"/> + <ref name="DCTnamespaceElements"/> + </choice> + <ref name="entity.noteLinkInfo"/> + </define> + <define name="termNoteGrp.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="termSec"> + <element name="termSec"> + <ref name="termSec.content"/> + <ref name="termSec.localattributes"/> + </element> + </define> + <define name="termSec.content"> + <ref name="term"/> + <choice> + <zeroOrMore> + <choice> + <ref name="termNote"/> + <ref name="termNoteGrp"/> + </choice> + </zeroOrMore> + <zeroOrMore> + <ref name="DCTnamespaceElements"/> + </zeroOrMore> + </choice> + <ref name="entity.auxInfo"/> + </define> + <define name="termSec.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="transac"> + <element name="transac"> + <ref name="transac.content"/> + <ref name="transac.localattributes"/> + </element> + </define> + <define name="transac.content"> + <text/> + </define> + <define name="transac.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">The + attribute value transactionType ensures that the content of the transac element will be + a transaction type.</a:documentation> + <ref name="transac.types"/> + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="transacGrp"> + <element name="transacGrp"> + <ref name="transacGrp.content"/> + <ref name="transacGrp.localattributes"/> + </element> + </define> + <define name="transacGrp.content"> + <choice> + <group> + <ref name="transac"/> + <zeroOrMore> + <choice> + <ref name="transacNote"/> + <ref name="date"/> + <ref name="note"/> + <ref name="ref"/> + <ref name="xref"/> + </choice> + </zeroOrMore> + </group> + <group> + <ref name="DCTnamespaceElements"/> + <zeroOrMore> + <choice> + <ref name="date"/> + <ref name="note"/> + <ref name="DCTnamespaceElements"/> + </choice> + </zeroOrMore> + </group> + </choice> + </define> + <define name="transacGrp.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="transacNote"> + <element name="transacNote"> + + <ref name="transacNote.content"/> + <ref name="transacNote.localattributes"/> + </element> + </define> + <define name="transacNote.content"> + <text/> + </define> + <define name="transacNote.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + <ref name="transacNote.types"/> + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="xref"> + <element name="xref"> + <ref name="xref.content"/> + <ref name="xref.localattributes"/> + </element> + </define> + <define name="xref.content"> + <text/> + </define> + <define name="xref.localattributes"> + <ref name="id.attributes"/> + <attribute name="target"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">The URI of + the external object.</a:documentation> + <data type="anyURI"> + <param name="pattern">https?://.+</param> + </data> + </attribute> + <attribute name="type"> + <ref name="xref.types"/> + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="tbx"> + <element name="tbx"> + <ref name="tbx.content"/> + <ref name="tbx.localattributes"/> + </element> + </define> + <define name="tbx.content"> + <ref name="tbxHeader"/> + <ref name="text"/> + </define> + <define name="tbx.localattributes"> + <attribute name="style"> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> Indicates + whether the file adheres to Data Category as Tag or Data Category as Attribute, DCT or + DCA, style. </documentation> + <choice> + <value>dca</value> + <value>dct</value> + </choice> + </attribute> + <attribute name="xml:lang"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the default language of the entire tbx element content. The allowed values of the + xml:lang attribute are found in IETF RFC 4646 or its successor, as indicated in IETF BCP + 47. This attribute is required for the tbx element.</a:documentation> + <text/> + </attribute> + <attribute name="type"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the type of tbx document. If the type attribute value TBX is used, then the TBX document + instance shall adhere to the default XCS file. If the TBX document instance adheres to + another XCS file, then the type attribute value can consist of TBX- plus another word + associated with the XCS file, such as 'TBX-Basic'.</a:documentation> + <data type="string"> + <param name="pattern">TBX-.+</param> + </data> + </attribute> + </define> + <define name="tbxHeader"> + <element name="tbxHeader"> + <ref name="tbxHeader.content"/> + <ref name="tbxHeader.localattributes"/> + </element> + </define> + <define name="tbxHeader.content"> + <ref name="fileDesc"/> + <optional> + <ref name="encodingDesc"/> + </optional> + <optional> + <ref name="revisionDesc"/> + </optional> + </define> + <define name="tbxHeader.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="p"> + <element name="p"> + + <ref name="p.content"/> + <ref name="p.localattributes"/> + </element> + </define> + <define name="p.content"> + <ref name="entity.noteText"/> + </define> + <define name="p.localattributes"> + <ref name="idlang.attributes"/> + <optional> + <attribute name="type"> + <text/> + </attribute> + </optional> + </define> + <define name="fileDesc"> + <element name="fileDesc"> + + <ref name="fileDesc.content"/> + <ref name="fileDesc.localattributes"/> + </element> + </define> + <define name="fileDesc.content"> + <optional> + <ref name="titleStmt"/> + </optional> + <optional> + <ref name="publicationStmt"/> + </optional> + <oneOrMore> + <ref name="sourceDesc"/> + </oneOrMore> + </define> + <define name="fileDesc.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="titleStmt"> + <element name="titleStmt"> + + <ref name="titleStmt.content"/> + <ref name="titleStmt.localattributes"/> + </element> + </define> + <define name="titleStmt.content"> + <ref name="title"/> + <zeroOrMore> + <ref name="note"/> + </zeroOrMore> + </define> + <define name="titleStmt.localattributes"> + <ref name="idlang.attributes"/> + </define> + <define name="title"> + <element name="title"> + + <ref name="title.content"/> + <ref name="title.localattributes"/> + </element> + </define> + <define name="title.content"> + <text/> + </define> + <define name="title.localattributes"> + <ref name="idlang.attributes"/> + </define> + <define name="publicationStmt"> + <element name="publicationStmt"> + + <ref name="publicationStmt.content"/> + <ref name="publicationStmt.localattributes"/> + </element> + </define> + <define name="publicationStmt.content"> + <oneOrMore> + <ref name="p"/> + </oneOrMore> + </define> + <define name="publicationStmt.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="sourceDesc"> + <element name="sourceDesc"> + <ref name="sourceDesc.content"/> + <ref name="sourceDesc.localattributes"/> + </element> + </define> + <define name="sourceDesc.content"> + <oneOrMore> + <ref name="p"/> + </oneOrMore> + </define> + <define name="sourceDesc.localattributes"> + <ref name="idlang.attributes"/> + </define> + <define name="encodingDesc"> + <element name="encodingDesc"> + + <ref name="encodingDesc.content"/> + <ref name="encodingDesc.localattributes"/> + </element> + </define> + <define name="encodingDesc.content"> + <oneOrMore> + <ref name="p"/> + </oneOrMore> + </define> + <define name="encodingDesc.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="revisionDesc"> + <element name="revisionDesc"> + + <ref name="revisionDesc.content"/> + <ref name="revisionDesc.localattributes"/> + </element> + </define> + <define name="revisionDesc.content"> + <oneOrMore> + <ref name="change"/> + </oneOrMore> + </define> + <define name="revisionDesc.localattributes"> + <ref name="idlang.attributes"/> + </define> + <define name="change"> + <element name="change"> + + <ref name="change.content"/> + <ref name="change.localattributes"/> + </element> + </define> + <define name="change.content"> + <oneOrMore> + <ref name="p"/> + </oneOrMore> + </define> + <define name="change.localattributes"> + <ref name="idlang.attributes"/> + </define> + <define name="text"> + <element name="text"> + + <ref name="text.content"/> + <ref name="text.localattributes"/> + </element> + </define> + <define name="text.content"> + <ref name="body"/> + <optional> + <ref name="back"/> + </optional> + </define> + <define name="text.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="body"> + <element name="body"> + + <ref name="body.content"/> + <ref name="body.localattributes"/> + </element> + </define> + <define name="body.content"> + <oneOrMore> + <ref name="conceptEntry"/> + </oneOrMore> + </define> + <define name="body.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="back"> + <element name="back"> + + <ref name="back.content"/> + <ref name="back.localattributes"/> + </element> + </define> + <define name="back.content"> + <zeroOrMore> + <ref name="refObjectSec"/> + </zeroOrMore> + </define> + <define name="back.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="refObjectSec"> + <element name="refObjectSec"> + + <ref name="refObjectSec.content"/> + <ref name="refObjectSec.localattributes"/> + </element> + </define> + <define name="refObjectSec.content"> + <oneOrMore> + <ref name="refObject"/> + </oneOrMore> + </define> + <define name="refObjectSec.localattributes"> + <ref name="id.attributes"/> + <attribute name="type"> + <text/> + </attribute> + </define> + <define name="refObject"> + <element name="refObject"> + <ref name="refObject.content"/> + <ref name="refObject.localattributes"/> + </element> + </define> + <define name="refObject.content"> + <oneOrMore> + <choice> + <ref name="itemSet"/> + <ref name="itemGrp"/> + <ref name="item"/> + </choice> + </oneOrMore> + </define> + <define name="refObject.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="item"> + <element name="item"> + + <ref name="item.content"/> + <ref name="item.localattributes"/> + </element> + </define> + <define name="item.content"> + <ref name="entity.noteText"/> + </define> + <define name="item.localattributes"> + <ref name="idtype.attributes"/> + </define> + <define name="itemGrp"> + <element name="itemGrp"> + + <ref name="itemGrp.content"/> + <ref name="itemGrp.localattributes"/> + </element> + </define> + <define name="itemGrp.content"> + <ref name="item"/> + <ref name="entity.noteLinkInfo"/> + </define> + <define name="itemGrp.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="itemSet"> + <element name="itemSet"> + + <ref name="itemSet.content"/> + <ref name="itemSet.localattributes"/> + </element> + </define> + <define name="itemSet.content"> + <oneOrMore> + <choice> + <ref name="item"/> + <ref name="itemGrp"/> + </choice> + </oneOrMore> + </define> + <define name="itemSet.localattributes"> + <ref name="idtype.attributes"/> + </define> + + + + <!-- DCA specific module attribute --> + <define name="dca.attributes"> + <optional> + <attribute name="module"> + <text/> + </attribute> + </optional> + </define> + + <!-- Extension Points for DCT --> + <define name="DCTnamespaceElements"> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> This is an + extension point for TBX data categories which are brought in from another namespace to form + a dialect. </documentation> + <element> + <anyName> + <except> + <nsName ns="urn:iso:std:iso:30042:ed-2"/> + </except> + </anyName> + <zeroOrMore> + <choice> + <attribute> + <anyName> + <except> + <nsName ns="urn:iso:std:iso:30042:ed-2"/> + </except> + </anyName> + </attribute> + <text/> + <ref name="DCTnamespaceElements"/> + </choice> + </zeroOrMore> + </element> + </define> + + <!-- Extension Points for DCA type values. If co-constraint validation is required, such constraints must be supplied via a Schematron file --> + <define name="admin.types"> + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in non-namespace environments (DCA style), replace + <text/> with the allowed values of the "type" attribute.</p> + </documentation> + <empty/> + </choice> + </define> + <define name="adminNote.types"> + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in non-namespace environments (DCA style), replace + <text/> with the allowed values of the "type" attribute.</p> + </documentation> + <empty/> + </choice> + </define> + <define name="descrip.types"> + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in non-namespace environments (DCA style), replace + <text/> with the allowed values of the "type" attribute.</p> + </documentation> + <empty/> + </choice> + </define> + <define name="descripNote.types"> + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in non-namespace environments (DCA style), replace + <text/> with the allowed values of the "type" attribute.</p> + </documentation> + <empty/> + </choice> + </define> + <define name="ref.types"> + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in non-namespace environments (DCA style), replace + <text/> with the allowed values of the "type" attribute.</p> + </documentation> + <empty/> + </choice> + </define> + <define name="transac.types"> + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in non-namespace environments (DCA style), replace + <text/> with the allowed values of the "type" attribute.</p> + </documentation> + <empty/> + </choice> + </define> + <define name="transacNote.types"> + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in non-namespace environments (DCA style), replace + <text/> with the allowed values of the "type" attribute.</p> + </documentation> + <empty/> + </choice> + </define> + <define name="xref.types"> + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in non-namespace environments (DCA style), replace + <text/> with the allowed values of the "type" attribute.</p> + </documentation> + <empty/> + </choice> + </define> + + <define name="termNote.types"> + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in non-namespace environments (DCA style), replace + <text/> with the allowed values of the "type" attribute.</p> + </documentation> + <empty/> + </choice> + </define> + + <start> + <ref name="tbx"/> + </start> +</grammar> diff --git a/reference-docs/schemas/TBX-Core_dialect/TBX-Core Definition.pdf b/reference-docs/schemas/TBX-Core_dialect/TBX-Core Definition.pdf new file mode 100644 index 0000000..08ec929 Binary files /dev/null and b/reference-docs/schemas/TBX-Core_dialect/TBX-Core Definition.pdf differ diff --git a/reference-docs/schemas/TBX-Linguist_dialect/DCA/Example_Astronomy_DCA_VALID.tbx b/reference-docs/schemas/TBX-Linguist_dialect/DCA/Example_Astronomy_DCA_VALID.tbx new file mode 100644 index 0000000..ccad346 --- /dev/null +++ b/reference-docs/schemas/TBX-Linguist_dialect/DCA/Example_Astronomy_DCA_VALID.tbx @@ -0,0 +1,4028 @@ +<?xml version="1.0" encoding="utf-8"?> +<?xml-model href="https://raw.githubusercontent.com/LTAC-Global/TBX-Linguist_dialect/master/DCA/TBXcoreStructV03_TBX-Linguist_integrated.rng" type="application/xml" schematypens="http://relaxng.org/ns/structure/1.0"?> +<?xml-model href="https://raw.githubusercontent.com/LTAC-Global/TBX-Linguist_dialect/master/DCA/TBX-Linguist_DCA.sch" type="application/xml" schematypens="http://purl.oclc.org/dsdl/schematron"?> +<tbx type="TBX-Linguist" style="dca" xml:lang="en" xmlns="urn:iso:std:iso:30042:ed-2"> + <tbxHeader> + <fileDesc> + <sourceDesc> + <p>TBX file, created via MultiTerm Export</p> + </sourceDesc> + </fileDesc> + </tbxHeader> + + <text> + <body> + <conceptEntry id="c1"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Galaxy_cluster#/media/File:Galaxy_cluster_IDCS_J1426.jpg">Open_Cluster.JPG</xref> + <note>G-Source: http://www.physics.drexel.edu/observatory/dump.shtml</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A group of stars formed together in the spiral + arms of a galaxy.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>open cluster</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">preferredTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">Over 1100 open clusters are known in our Milky + Way Galaxy, and this is probably only a small percentage of the + total population which is probably some factor higher; estimates of + as many as about 100,000 Milky Way open clusters have been given. </descrip> + <admin type="source">http://seds.org/MESSIER/open.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>galactic cluster</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">supersededTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">In contrast, the galactic cluster represented by + M29 is a grouping of stars—a “knot” of stars in the stellar + backdrop.</descrip> + <admin type="source">http://www.eastbayastro.org/2000/0900/r0900-8.htm</admin> + </descripGrp> + <note>Another name for an open star cluster. They are often termed Galactic + Clusters because they are found mainly in the plane of our galaxy. If + you were to view our galaxy from afar, you would find that all the + open/galactic clusters lie within the spiral arms of the galaxy.</note> + <note>N-Source: + http://www.delscope.demon.co.uk/astronomy/glossary.htm#G</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una acumulación de una docena hasta varios miles + de jóvenes estrellas en el plano de las galaxias.</descrip> + <admin type="source">http://www.espacioprofundo.com.ar/diccionario/Glosario_de_Astronomia/vertermino/Cumulo_abierto.html</admin> + </descripGrp> + <termSec> + <term>cúmulo abierto</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">M7 es uno de los cúmulos abiertos estelares más + prominentes del cielo. El cúmulo, dominado por brillantes estrellas + azules, puede ser visto a ojo desnudo en un cielo oscuro en la cola + de la constelación del Escorpión (Scorpius).Contiene unas 100 + estrellas en total, tiene una edad aproximada de 200 millones de + años, mide 25 años luz de ancho, y se encuentra a unos 1000 años luz + de distancia.</descrip> + <admin type="source">http://observatorio.info/2009/11/m7-cumulo-abierto-en-scorpius-2/</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c2"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Accretion_disk#/media/File:Star_with_accretion_disk.jpg">Accretion_Disk.jpg</xref> + <note>G-Source: + http://www.cfht.hawaii.edu/Instruments/Spectroscopy/Espadons/www.ast.obs-mip.fr/users/donati/press/fuori_eng.html</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A structure that forms around a compact object + (e.g. a white dwarf, neutron star, or black hole) when matter flows + towards it.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>circumstellar accretion disk</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">preferredTerm-admn-sts</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">In contrast with the violence of merging, the + gradual growth of massive stars by accretion is likely to produce + less infrared variability, relatively thin circumstellar accretion + disks that maintain their orientation, and collimated bipolar + outflows that are scaled-up versions of those produced by low-mass + young stellar objects.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + <termSec> + <term>accretion disc</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">Accretion Disc Evolution in Single and Binary T + Tauri Stars</descrip> + <admin type="source">http://cdsweb.cern.ch/record/369655</admin> + </descripGrp> + </termSec> + <termSec> + <term>circumstellar disk</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">Our results suggest a scenario of a central star + accreting material from a circumstellar disc at the centre of a cool + extended rotating torus, while driving a fast bipolar wind. </descrip> + <admin type="source">http://adsabs.harvard.edu/abs/2010MNRAS.402.1504D</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una estructura en forma de disco alrededor de un + objeto central masivo que alimenta el cuerpo central siendo atraido por + éste y contribuye a su aumento de masa.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Disco_de_acreci%C3%B3n</admin> + </descripGrp> + <termSec> + <term>disco de acreción</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">preferredTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">Lo que alimenta esta actividad es el gas + extraído de la estrella normal, que, cayendo en espiral hacia el + agujero negro, se acumula en un denso disco de acreción.</descrip> + <admin type="source">http://www.amazings.com/ciencia/noticias/010210e.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>disco de acrecimiento</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">Imágenes de estrellas jóvenes con discos de + acrecimeinto y chorros colimados de material, tomadas con el + telescopio espacial Hubble.</descrip> + <admin type="source">http://www.laeff.inta.es/index.php?op=modload&name=phpWiki&file=index&pagename=Research-Brown%20Dwarfs-BD_esp-DiscosAcrecimiento</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c3"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Black_hole#/media/File:BH_LMC.png">Black_Hole.jpg</xref> + <note>G-Source: http://wallpaper-s.org/12__Supermassive_Black_Hole.htm</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A region of space where the gravitational force + is so strong that not even light can escape from it.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>black hole</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">As matter spirals toward and into the black + hole, some of its gravitational potential energy may be efficiently + converted into relativistic jets launched by the magnetic field + along the spin axis.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un punto super-denso en el espacio formado por el + colapso de una estrella donde nada puede escapar de su influencia + gravitacional. </descrip> + <admin type="source">www.atlasoftheuniverse.com/espanol/glossary.html</admin> + </descripGrp> + <termSec> + <term>agujero negro</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">En teoría un agujero negro se origina hacia el + final de la vida de una estrella, cuando ésta se contrae mas allá de + un límite determinado - conocido como radio de Schwarzschild - y se + hace más pequeña y mas densa que una estrella de neutrones, tanto + que ni la luz puede escapar de su campo gravitatorio.</descrip> + <admin type="source">http://html.rincondelvago.com/agujeros-negros_5.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c4"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Gamma-ray_burst#/media/File:GRB080319B_illustration_NASA.jpg">Gamma_Ray_Burst.jpg</xref> + <note>G-Source: + http://nakedmaninthetree.wordpress.com/2009/02/22/galaxies-and-the-future/</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A temporary intese burst of gamma rays and X-rays + from a cosmic source.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>gamma-ray burst</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">The extremely rare merger of two stars close to + the upper-mass end of the initial mass function may be a possible + pathway to hypernova-generated gamma-ray bursts.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + <termSec> + <term>GRB</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">acronym</termNote> + <descripGrp> + <descrip type="context">The off-axis collisions and merging of stars + near the top of the stellar mass spectrum may result in the + production of GRBs.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Destellos de rayos gamma que pueden durar desde + unos nanosegundos hasta cerca de una hora.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Brote_de_rayos_gamma</admin> + </descripGrp> + <termSec> + <term>explosión de rayos gamma</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Una poderosa explosión de rayos gamma, detectada + el 19 de marzo por el satélite Swift, de la NASA, batió el récord + como el objeto más distante que se pudo observar a simple + vista.</descrip> + <admin type="source">http://ciencia.nasa.gov/headlines/y2008/21mar_nakedeye.htm</admin> + </descripGrp> + </termSec> + <termSec> + <term>brote de rayos gamma</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">John Ellis (entrevistado por Punset en su + despacho en el CERN en un programa de Redes) y sus colaboradores + mostraron cómo utilizar las propiedades de los grandes brotes de + rayos gamma (gamma-ray bursters o GRBs) para responder a esta + cuestión.</descrip> + <admin type="source">http://francisthemulenews.wordpress.com/2009/02/21/el-mayor-brote-de-rayos-gamma-grb-080916c-acerca-la-gravedad-cuantica-al-mundo-de-planck/</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c5"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Globular_cluster#/media/File:A_Swarm_of_Ancient_Stars_-_GPN-2000-000930.jpg">Globular_Cluster.jpg</xref> + <note>G-Source: http://www.astrographics.com/GalleryPrintsIndex/GP0046.html</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A roughly spherical group of old stars in the + halo of the galaxy.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>globular cluster</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Although the standard accretion scenario may + well explain the formation of most massive stars, the existence of + blue stragglers in globular clusters indicates that mergers do occur + in nature.</descrip> + <admin type="source">Birth of High-Mass Stars</admin> + </descripGrp> + <note>Related Term: star cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un tipo de cúmulo estelar que consiste en una + agrupación de miles de estrellas viejas, gravitacionalmente ligadas, con + distribución aproximadamente esférica, y que orbita en torno a una + galaxia de manera similar a un satélite.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/C%C3%BAmulo_globular</admin> + </descripGrp> + <termSec> + <term>cúmulo globular</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context"> De los 200 cúmulos globulares que sobreviven + hoy, M3 es uno de los más grande y luminoso, fácilmente observable + con binoculares en el hemisferio Norte del cielo.</descrip> + <admin type="source">http://www.tayabeixo.org/portadas/m3.htm</admin> + </descripGrp> + <note>Related Term: cúmulo estelar</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c6"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Main_sequence#/media/File:HRDiagram.png">Main_Sequence.jpg</xref> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: http://www.skyofplenty.com/?page_id=374</note> + <descripGrp> + <descrip type="definition">Of or dealing with a major group of stars forming + a band stretching from upper left to lower right on a + Hertzsprung-Russell diagram when being plotted by luminosity and surface + temperature.</descrip> + <admin type="source">http://en.wiktionary.org/wiki/main-sequence</admin> + </descripGrp> + <termSec> + <term>main-sequence</term> + + + <termNote type="partOfSpeech">adjective</termNote> + <descripGrp> + <descrip type="context">However, immediately after its formation, the + merger product is likely to have a photospheric radius considerably + larger than that of a main-sequence star with the same + mass.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Pertenece a las estrellas en la región del + diagrama de Hertzsprung-Russell en la que se encuentran la mayor parte + de las estrellas que transforman hidrógeno en helio.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Secuencia_principal</admin> + </descripGrp> + <termSec> + <term>de secuencia principal</term> + + + <termNote type="partOfSpeech">adjective</termNote> + <descripGrp> + <descrip type="context">Por ejemplo, nuestro sol es una estrella de + secuencia principal regular de tamaño pequeño. </descrip> + <admin type="source">http://celestia.albacete.org/celestia/celestia/stars/secu5.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c7"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Protostar#/media/File:A_diamond_in_the_dust.jpg">Protostar.JPG</xref> + <note>G-Source: http://www.konkoly.hu/KISAG/Science/star/star_intro.html</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A star in the earliest observable stage of + formation.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>protostar</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Alternatively, it has been suggested that + massive stars form from the merging of lower mass protostars in + high-density protostar clusters (Bonnell et al.1998; Stahler et al. + 2000; Bonnell 2002; Zinnecker & Bate 2002).</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: + http://geocities.ws/acarvajaltt/temas/estrellas_nacimiento_estelar.html</note> + <descripGrp> + <descrip type="definition">Una región muy densa o descorazonada de nubes + moleculares donde existen estrellas en proceso de formación.</descrip> + <admin type="source">www.astrocosmo.cl/glosario/glosar-p.htm</admin> + </descripGrp> + <termSec> + <term>protoestrella</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">En estos primeros estadios, la protoestrella es + un objeto muy activo, y produce un viento bipolar formado por dos + chorros opuestos de material de alta velocidad. </descrip> + <admin type="source">http://www.fomento.es/MFOM/LANG_CASTELLANO/DIRECCIONES_GENERALES/INSTITUTO_GEOGRAFICO/Astronomia/InvestermSecacion/astronomia/protoestrellas.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c8"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Star_cluster#/media/File:M92_arp_750pix.jpg">Star_Cluster.jpg</xref> + <note>G-Source: http://apod.nasa.gov/apod/ap060109.html</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A collection of stars formed together from the + same gas cloud and bound together by mutual gravitational + attraction.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>star cluster</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Most star clusters are too far away and the + white dwarfs are too faint to be seen by ground-based telescopes, + but Hubble's powerful vision sees many of them.</descrip> + <admin type="source">http://hubblesite.org/newscenter/archive/releases/star%20cluster/2008/25/full/</admin> + </descripGrp> + <note>Related Term: globular cluster</note> + <note>Related Term: open cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un grupo de estrellas atraídas entre sí por su + gravedad mutua.</descrip> + <admin type="source">http://iopscience.iop.org/1538-3881/129/5/2281/pdf/1538-3881_129_5_2281.pdf</admin> + </descripGrp> + <termSec> + <term>cúmulo estelar</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">preferredTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">“Es como encontrar un pez fuera del agua”, dice + Ed Churchwell, profesor de astronomía de la Universidad de + Wisconsin-Madison, quien con un equipo de científicos de UW-Madison, + de la Universidad de Wyoming, de la Universidad de Boston, del + Instituto de Ciencia Espacial de Boulder, Colorado, y del Centro de + Ciencia Spitzer descubrieron este inusual cúmulo estelar con la + ayuda del Telescopio Espacial Spitzer de la NASA. </descrip> + <admin type="source">http://www.astroseti.org/vernew.php?codigo=1117</admin> + </descripGrp> + </termSec> + <termSec> + <term>cúmulo de estrellas</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">Los cúmulos de estrellas se clasifican en dos + grupos: cúmulos abiertos, que no poseen forma definida, y cúmulos + globulares, que son esféricos o casi esféricos.</descrip> + <admin type="source">http://www.astromia.com/universo/cumulos.htm</admin> + </descripGrp> + <note>Related Term: cúmulo globular</note> + <note>Related Term: cúmulo abierto</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c9"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Milky_Way#/media/File:ESO-VLT-Laser-phot-33a-07.jpg">Milky_Way.jpg</xref> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: http://www.cfa.harvard.edu/~afrebel/milky-way-2.jpg</note> + <descripGrp> + <descrip type="definition">A band of faint light across the sky, visible to + the naked eye on a moonless night, consisting of stars and glowing gas + in the disk of our own Galaxy.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>Galaxy</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">If merging is an important pathway to the + formation of massive stars, then it is expected that some + highluminosity IRAS sources in our Galaxy have brightened or faded + since the IRAS observations were made.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + <termSec> + <term>Milky Way Galaxy</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">fullForm</termNote> + </termSec> + <termSec> + <term>Milky Way</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: http://oacs-unah.edu.hn/an111/vrt/img/via_lactea.jpg</note> + <descripGrp> + <descrip type="definition">Una galaxia espiral en la que se encuentra el + Sistema Solar y, por ende, la Tierra.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Vía_Láctea</admin> + </descripGrp> + <termSec> + <term>Galaxia</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">La Vía Láctea, también llamada la Galaxia, es un + agrupamiento de estrellas con forma de disco, que incluye al Sol y a + su sistema solar.</descrip> + <admin type="source">www.todoelsistemasolar.com.ar/vlactea.htm</admin> + </descripGrp> + </termSec> + <termSec> + <term>Vía Láctea</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">La Via Láctea és una galaxia grande, espiral y + puede tener unos 100.000 millones de estrellas, entre ellas, el Sol. </descrip> + <admin type="source">http://www.astromia.com/universo/vialactea.htm</admin> + </descripGrp> + </termSec> + <termSec> + <term>galaxia Vía Láctea</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">La galaxia Vía Láctea es una galaxia espiral que + es nuestro hogar, al igual que el de otras 100 mil millones + estrellas. </descrip> + <admin type="source">http://www.windows.ucar.edu/tour/link=/the_universe/Milkyway.sp.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c10"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Star#/media/File:The_Sun_by_the_Atmospheric_Imaging_Assembly_of_NASA%27s_Solar_Dynamics_Observatory_-_20100819.jpg">Star.jpg</xref> + <note>G-Source: + http://lh4.ggpht.com/_EuutPdvjcY0/SQ2jGBKWO7I/AAAAAAAAALM/gjDMVimDQc8/005Est.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A large, luminous ball of gas generating energy + internally by nuclear fusion.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>star</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">While the behavior of stars forming by accretion + is reasonably well understood,the consequences of merging have not + been fully investermSecated.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una enorme y densa bola de gas que genera fusión + nuclear, liberando así una gran cantidad de energía</descrip> + <admin type="source">spaceplace.nasa.gov/sp/kids/spitzer/signs/sign_glossary.shtml</admin> + </descripGrp> + <termSec> + <term>estrella</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Las estrellas son enormes aglomeraciones de gas, + principalmente Hidrogeno, cuya temperatura es tan alta debido a la + fusión de este elemento, que irradian luz a lo largo de todo el + espectro electromagnético. Poseen diferentes temperaturas que varían + desde los 2000 grados Celsius hasta los 50000.</descrip> + <admin type="source">http://www.astrosurf.com/astronosur/estrellas.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c11"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Ultraviolet#/media/File:UV_LED_Fluoresence.jpg">UV_Radiation.jpg</xref> + <note>G-Source: http://drdima.files.wordpress.com/2009/05/sun-rays.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The region of the electromagnetic spectrum + spanning the wavelength range from the Lymann limit at 91.2 nm to 350 + nm.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>UV radiation</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">UV radiation from stars and shocks likely + provide the minimum level of ionization required to couple these + fields strongly to the entangled medium.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + <termSec> + <term>ultraviolet radiation</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">Ultraviolet (UV) radiation is part of the + electromagnetic spectrum emitted by the sun. </descrip> + <admin type="source">http://www.who.int/uv/en/</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">La radiación electromagnética cuya longitud de + onda está comprendida aproximadamente entre los 400 nm y los 15 + nm.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Radiaci%C3%B3n_UV</admin> + </descripGrp> + <termSec> + <term>radiación UV</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">Los usuarios de camas solares se someten a dosis + considerables de radiaciones UV artificiales para conseguir un + bronceado complementario al obtenido al tomar el sol.</descrip> + <admin type="source">http://copublications.greenfacts.org/es/camas-solares/</admin> + </descripGrp> + </termSec> + <termSec> + <term>radiación ultravioleta</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">La radiación ultravioleta se encuentra entre la + luz visible y los rayos X del espectro electromagnético.</descrip> + <admin type="source">http://www.windows.ucar.edu/tour/link=/physical_science/magnetism/em_ultraviolet.sp.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c12"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Magnetic_field#/media/File:VFPt_magnets_BHM.svg">Magnetic_Field.jpg</xref> + <note>G-Source: http://www.greatdreams.com/magnet1.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A region subject to the influence of magnetism + that is manifested by the mechanical forces that it exerts upon + electricity moving across it and upon the poles of magnets placed in + it.</descrip> + <admin type="source">Merriam-Webster2002</admin> + </descripGrp> + <termSec> + <term>magnetic field</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Detailed consideration of the merger process + will require numerical modeling in which the hydrodynamics, effects + of gravity,magnetic fields, and radiation are considered + carefully.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un campo de fuerza creado como consecuencia del + movimiento de cargas eléctricas, del flujo de la electricidad.</descrip> + <admin type="source">http://www.greenfacts.org/es/glosario/abc/campo-magnetico.htm</admin> + </descripGrp> + <termSec> + <term>campo magnético</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">El campo magnético es producido por la corriente + eléctrica que circula por un conductor.</descrip> + <admin type="source">http://teleformacion.edu.aytolacoruna.es/FISICA/document/teoria/A_Franco/elecmagnet/magnetico/cMagnetico.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c13"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Blue_straggler#/media/File:Ngc6397_hst_blue_straggler.jpg">Blue_Straggler.jpg</xref> + <note>G-Source: http://images.spaceref.com/news/2009/ooBlue_Straggler09.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A blue main-sequence star, usually found in a + globular or open cluster that appears to be slower in its evolution than + other stars of similar mass and luminosity in the same + cluster.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>blue straggler</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Numerical models of stellar collisions leading + to the formation of blue stragglers in globular clusters (Lombardi + et al. 2002, 2003; Fregeau et al. 2004) indicate that merger + products have radii up to 30 times larger than that of an equivalent + main-sequence star.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Estrellas que aparentan una edad menor que la del + sistema estelar al que pertenecen, si se supone que se formaron junto + con él.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Estrella_rezagada_azul</admin> + </descripGrp> + <termSec> + <term>estrella rezagada azul</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">preferredTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">Las últimas observaciones de las “rezagadas + azules”, estrellas atípicas que aparentan ser más jóvenes que el + sistema estelar al que pertenecen, han proporcionado dos modelos + diferentes sobre su origen.</descrip> + <admin type="source">http://mundoastronomia.portalmundos.com/nuevas-pistas-sobre-el-origen-de-las-estrellas-rezagadas-azules/</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c14"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The sudden collapse of a massive star when the + internal pressure pushing outwards falls so that it cannot balance the + weight of material pressing inward.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>gravitational collapse</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Stars form from the gravitational collapse of + turbulent molecular cloud cores (Elmegreen & Scalo 2004; Mac Low + & Klessen 2004).</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El estado final de la evolución de una estrella + de gran masa en el que la materia se comprime bajo la acción de su + propia atracción gravitatoria, con desprendimiento de grandes cantidades + de energía.</descrip> + <admin type="source">http://www.conocimientosweb.net/portal/term6172.html</admin> + </descripGrp> + <termSec> + <term>colapso gravitacional</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Esto sucede si la masa de un pedazo de la nube + excede cierto valor crítico, de modo tal que la fuerza de gravedad + vence definitivamente y el pedazo empieza a contraerse, aumentando + su densidad. Este proceso se llama colapso gravitacional. </descrip> + <admin type="source">http://bibliotecadigital.ilce.edu.mx/sites/ciencia/volumen1/ciencia2/06/html/sec_15.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c15"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Binary_star#/media/File:Algol_AB_movie_imaged_with_the_CHARA_interferometer_-_labeled.gif">Binary_Star.jpg</xref> + <note>G-Source: + http://lh6.ggpht.com/_6hgSmco4R9M/SaqplXGqJfI/AAAAAAAAA1k/B3a43_O9VI8/56_Binary_Stars_thumb3.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A pair of stars in orbit around each other, held + together by the graviational attraction between them.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>binary star</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">These authors considered collision partners + having similar masses and concluded that such interactions can at + most account for a small fraction of the observed binary star + population in young clusters.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un sistema estelar compuesto de dos estrellas que + orbitan mutuamente alrededor de un centro de masas común.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Estrella_binaria</admin> + </descripGrp> + <termSec> + <term>estrella binaria</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">La explosión de una estrella binaria dentro de + una nebulosa planetaria ha sido capturado por un equipo dirigido por + investermSecadores del University College of London UCL - es un + acontecimiento que no ha sido presenciado hace más de 100 + años.</descrip> + <admin type="source">http://www.astroelche.es/blog/index.php?blog=2&title=astronomos-capturam-la-explosion-de-una-&more=1&c=1&tb=1&pb=1</admin> + </descripGrp> + </termSec> + <termSec> + <term>estrella doble</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">preferredTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">Una estrella doble es una pareja de estrellas + que se mantienen unidas por la fuerza de la gravitación y giran en + torno a su centro común.</descrip> + <admin type="source">http://www.astromia.com/universo/dobles.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c16"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Initial_mass_function#/media/File:LH_95.jpg" + >Initial_Mass_Function.JPG</xref> + <note>G-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <note>This figure compares the IMFs by ploting mass fraction per dex versus mass, + i.e., normalized so that the integral under each curve is unity. They are + assumed to be valid from 0.1 to 120 solar masses.</note> + <note>N-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A mathematical description of the relative + frequncy with which stars of various masses are formed.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>initial mass function</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The extremely rare merger of two stars close to + the upper-mass end of the initial mass function may be a possible + pathway to hypernova-generated gamma-ray bursts.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">La expresión numérica que determina el número de + estrellas con masa en un rango determinado.</descrip> + <admin type="source">Basado en http://laeff.cab.inta-csic.es/modules.php?op=modload&name=phpWiki&file=index&pagename=Research-Estrellas-IMF</admin> + </descripGrp> + <termSec> + <term>función inicial de masa</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Estado evolutivo y función inicial de masa de + cúmulos jóvenes en la gran nube de Magallanes (estudio en el + ultravioleta).</descrip> + <admin type="source">http://dialnet.unirioja.es/servlet/tesis?codigo=11651</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c17"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <termSec> + <term>Bally2005</term> + + + <note>Author[s]: Bally, John and Hans Zinnecker</note> + <note>Journal Title: The Astronomical Journal</note> + <note>Article Title: The Birth of High-Mass Stars: Accertion and/or + Mergers?</note> + <note>Volume: 129</note> + <note>Publication Place: U.S.A.</note> + <note>Publisher: The American Astronomical Society</note> + <note>Publication Year: May 2005</note> + <note>Page(s): 2281-2293</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c18"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <termSec> + <term>Cambridge2007</term> + + + <note>Author[s]: Mitton, Jaqueline</note> + <note>Book Title: Cambridge Illustrated Dictionary of Astronomy</note> + <note>Publication Place: New York</note> + <note>Publisher: Cambridge University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c19"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <termSec> + <term>Merriam-Webster2002</term> + + + <note>Book Title: Webster's Third New International Dictionary</note> + <note>Editor[s]: Gove, Philip Babcock</note> + <note>Volume: Third Edition</note> + <note>Publication Place: Springfield, Massachusetts</note> + <note>Publisher: Merriam-Webster INC.</note> + <note>Publication Year: 2002</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c20"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <termSec> + <term>Oxford2007</term> + + + <note>Book Title: Oxford Dictionary of Astronomy</note> + <note>Editor[s]: Ridpath, Ian</note> + <note>Volume: Second Edition</note> + <note>Publication Place: New York</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c21"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Supernova#/media/File:SN1994D.jpg">Supernova.jpg</xref> + <note>G-Source: + http://jcconwell.wordpress.com/2009/07/24/top-10-ways-the-universe-could-kill-us/supernova/</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A catastrophic stellar explosion in which so much + energy is released that the supernova alone can outshine an entire + galaxy of billions of stars.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>supernova</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The supermassive object may be eventually + disrupted by an unusually violent supernova explosion (a hypernova) + soon after formation.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una estrella que estalla y lanza a todo su + alrededor la mayor parte de su masa a altísimas velocidades.</descrip> + <admin type="source">http://www.astromia.com/glosario/supernova.htm</admin> + </descripGrp> + <termSec> + <term>supernova</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Un equipo de científicos británicos propone esta + semana en la revista Nature que la tenue supernova SN2008ha, + descubierta por una adolescente estadounidense en noviembre de 2008, + podría ser la explosión de una estrella masiva, en lugar de proceder + de una enana blanca como se planteaba hasta ahora.</descrip> + <admin type="source">http://www.plataformasinc.es/index.php/esl/Noticias/Una-supernova-observada-por-astronomos-aficionados-abre-el-debate-entre-los-profesionales</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c22"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <termSec> + <term>Moore2003</term> + + + <note>Author[s]: Moore, Patrick</note> + <note>Book Title: Philip's Atlas of the Universe</note> + <note>Publication Place: Heron Quays, London</note> + <note>Publisher: Philip's</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c23"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Red_giant#/media/File:Mira_1997.jpg">Red_Giant.jpg</xref> + <note>G-Source: + http://www.lcsd.gov.hk/CE/Museum/Space/EducationResource/Universe/framed_e/lecture/ch15/imgs/red_size.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A cool, large and highly luminous star that has + left the main sequence and is powered by heavier elements than + hydrogen.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>red giant</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The core temperature becomes so high that helium + start to 'burn', producing carbon; around this active core there is + a shell where hydrogen is still producing energy. The star becomes + unstable, and the outer layers swell out, cooling as they do so. The + star becomes a red giant.</descrip> + <admin type="source">Moore2003</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una estrella de masa baja o intermedia (menos de + 8-9 masas solares) que, tras haber consumido el hidrógeno en su núcleo + durante la etapa de secuencia principal, convirtiéndolo en helio por + fusión nuclear, comienza a quemar hidrógeno en una cáscara alrededor del + núcleo de helio inerte.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Gigante_roja</admin> + </descripGrp> + <termSec> + <term>gigante roja</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">La gigante roja S Orionis (S Ori) es una + estrella variable del tipo Mira. Su masa es similar a la del Sol, + con la diferencia de que está mucho más cerca de convertirse en una + enana blanca, el mismo final que le espera a nuestro Sol dentro de 5 + mil millones de años.</descrip> + <admin type="source">http://www.solociencia.com/astronomia/07071709.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c24"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Red_dwarf#/media/File:New_shot_of_Proxima_Centauri,_our_nearest_neighbour.jpg">Red_Dwarf.jpg</xref> + <note>G-Source: http://www.wolflodge.org/bluestar/h_red_dwarf_02.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A cool, faint, low-mass star lying at the lower + end of the main sequence of spectral type K or M.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>red dwarf</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The dim red dward Proxima, more than a degree + away from Alpha, is slightly closer to us.</descrip> + <admin type="source">Moore2003</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una estrella pequeña y relativamente fría de la + secuencia principal, ya sea de tipo espectral K tardío o M.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Enana_roja</admin> + </descripGrp> + <termSec> + <term>enana roja</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">El planeta que se ha descubierto girando + alrededor de esta enana roja tiene una masa equivalente a la de + Neptuno, es decir, es sólo 17 veces mayor que la Tierra y mucho + menor que Saturno.</descrip> + <admin type="source">http://axxon.com.ar/not/157/c-1570034.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c25"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Stellar_classification#/media/File:Zeta_Puppis.png">Spectral_Type.jpg</xref> + <note>G-Source: + http://www.astro.columbia.edu/~archung/labs/spring2002/images/spectral_type2.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A means of classifying stars according to the + details of their spectrum, depending largely on their surface + temperature.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>spectral type</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">In this version of a typical HR diagram, the + stars are plotted according to their spectral types and suface + temperatures (horzontal axis, x) and their luminositites in therms + of the Sun (vertical axis, y).</descrip> + <admin type="source">Moore2003, 171</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El espectro de una estrella clasificado por una + letra (O, B, A, F, G, K, M, R, N, S) seguida de un digito que describe + el color de la estrella y su temperatura.</descrip> + <admin type="source">Basado en http://www.espacioprofundo.com.ar/diccionario/Glosario_de_Astronomia/vertermino/Tipo_espectral.html</admin> + </descripGrp> + <termSec> + <term>tipo espectral</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">En el gráfico superior se muestra la intensidad + de las líneas espectrales según la temperatura de la estrella (tipo + espectral)</descrip> + <admin type="source">http://www.astrosurf.com/astronosur/estrellas.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c26"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/White_dwarf#/media/File:Sirius_A_and_B_Hubble_photo.editted.PNG">White_Dwarf.jpg</xref> + <note>G-Source: http://www.stsci.edu/~inr/thisweek1/thisweek/WhiteDwarf.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A small dense star that is has run out of fuel + for nuclear fusion, collapsing under its own gravity and blowing off its + outer layers to form a planetary nebula in the process.</descrip> + <admin type="source">Based on Oxford2007 and Cambridge2007</admin> + </descripGrp> + <note>This is the end-result of all but the most massive of stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>white dwarf</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">To the upper right lie giants and supergiants of + tremendous luminosity, while to the lower left there are the white + dwarfs, which are in a differnt category and were not known when HR + Diagrams were introduced.</descrip> + <admin type="source">Moore2003, 170</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un remanente estelar que se genera cuando una + estrella de masa menor a 9-10 masas solares ha agotado su combustible + nuclear.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Enana_blanca</admin> + </descripGrp> + <termSec> + <term>enana blanca</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Cuando el material fusionable se agota la + estrella pierde la presión interna producida por la fusión nuclear y + puede colapsar inmediatamente terminando en una enana + blanca.</descrip> + <admin type="source">http://astroverada.com/_/Main/T_evolucion.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c27"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Planetary_nebula#/media/File:NGC6543.jpg">Planetary_Nebula.jpg</xref> + <note>G-Source: + http://www.phys.ncku.edu.tw/~astrolab/mirrors/apod_e/image/0901/ngc2818_hheritage_800.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A bright cloud of glowing gas and dust + surrounding a highly evolved star.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <note>As mass is gradually lost, the core of the star becomes more exposed, + ultimately becoming a white dwarf. Also, planetary nebulae have nothing to + do with planets, and are not true nebulae.</note> + <note>N-Source: Based on Oxford2007 and Moore2003, 186</note> + <termSec> + <term>planetary nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The star's outer layers are thrown off, and for + a cosmically brief period - no more than about 100,000 years - we + have the phenomenon of what is termed a planetary nebula.</descrip> + <admin type="source">Moore2003, 173</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una nebulosa de emisión consistente en una + envoltura brillante en expansión de plasma y gas ionizado, expulsada + durante la fase de rama asintótica gigante que atraviesan las estrellas + gigantes rojas en los últimos momentos de sus vidas.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Nebulosa_planetaria</admin> + </descripGrp> + <termSec> + <term>nebulosa planetaria</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Las nebulosas planetarias resultan objetos muy + espectaculares si se observan con un telescopio de media o gran + potencia.</descrip> + <admin type="source">http://www.astromia.com/glosario/nebulosaplanetaria.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c28"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Emission_nebula#/media/File:Ring_Nebula.jpg">Emission_Nebula.jpg</xref> + <note>G-Source: http://apod.nasa.gov/apod/image/0612/NGC2174_lrg.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A luminous cloud of gas and sust in space which + shines with its own light, which can be generated in several + ways.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <note>Ultraviolet radiation, gas cloud collisions, and synchrotron radiation can + all cause the emission nebula to shine.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>emission nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">preferredTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">In this and other similar emission nebulae, + energetic ultraviolet light from a hot young star strips electrons + from the surrounding hydrogen atoms.</descrip> + <admin type="source">http://apod.nasa.gov/apod/emission_nebulae.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una nube de gas interestelar que brilla por la + excitación del gas, causado por radiación ultravioleta emitida por + estrellas inmersas en la nube o por calentamiento debido a otro + mecanismos. </descrip> + <admin type="source">http://www.diclib.com/Nebulosa%20de%20emisi%C3%B3n/show/en/es_astronomia/726</admin> + </descripGrp> + <termSec> + <term>nebulosa de emisión</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Las nebulosas de emisión estan normalmente en + los lugares de formación de estrellas.</descrip> + <admin type="source">http://www.astrored.net/nebulosaweb/types.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c29"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Nebula#/media/File:Eagle_nebula_pillars.jpg">Nebula.jpg</xref> + <note>G-Source: + http://my-blackberry.net/wallpapers/49/m/NASA_-_The_Horsehead_Nebula%2C_B33%2C_Orion_Nebula.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A cloud of interstellar gas and dust.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <note>The term was originally applied to any object with a fuzzy telescopic + appearance, but with the advent of larger instruments many 'nebulae' were + found to consist of faint stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <note>Grammatical Number: singular</note> + <descripGrp> + <descrip type="context">According to current theory, a star begins by + condensing out of the tenuous material making up a nebula.</descrip> + <admin type="source">Moore2003, 172</admin> + </descripGrp> + </termSec> + <termSec> + <term>nebulae</term> + + + <termNote type="partOfSpeech">noun</termNote> + <note>Grammatical Number: plural</note> + <descripGrp> + <descrip type="context">Other nebulae are within the range of small + telescopes.</descrip> + <admin type="source">Moore2003, 187</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Regiones del medio interestelar constituidas por + gases (principalmente hidrógeno y helio) y polvo.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Nebulosa</admin> + </descripGrp> + <termSec> + <term>nebulosa</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">A unos 1.500 años-luz de distancia, dentro de + nuestro brazo espiral en la Vía Láctea, la Nebulosa de Orión está en + el centro de la región de la Espada de la constelación de Orión el + Cazador, que domina el cielo nocturno a inicios del invierno, en las + latitudes Norte.</descrip> + <admin type="source">http://www.oarval.org/OrionNebsp.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c30"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Dark_nebula#/media/File:All_Quiet_in_the_Nursery%3F.jpg">Dark_Nebula.jpg</xref> + <note>G-Source: http://www.mallorcaweb.net/masm/obstel/caballo.GIF</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A type of interstellar cloud that is so dense + that it obscures the light from the background emission or reflection + nebula or that it blocks out background stars.</descrip> + <admin type="source">http://en.wikipedia.org/wiki/Dark_nebula</admin> + </descripGrp> + <termSec> + <term>dark nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">preferredTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">There is no difference between a dark nebula and + a bright one, except for the lack of illumination.</descrip> + <admin type="source">Moore2003, 187</admin> + </descripGrp> + </termSec> + <termSec> + <term>absorbtion nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">An absorption nebula is a dense cloud of dust + and gas. From the point of view of an observer on Earth, it absorbs + the light from more distant stars, creating a dark, starless + region.</descrip> + <admin type="source">http://www.glyphweb.com/esky/concepts/absorptionnebula.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Nubes de polvo que simplemente tapan la luz de lo + que haya detras.</descrip> + <admin type="source">http://www.astrored.net/nebulosaweb/types.html</admin> + </descripGrp> + <termSec> + <term>nebulosa oscura</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">preferredTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">Aqui hay un mapa que muestra las regiones de + nebulosas oscuras que estan en un radio de 2000 años luz.</descrip> + <admin type="source">http://www.atlasoftheuniverse.com/espanol/darknebs.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>nebulosa de absorción</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">El caso más opuesto a las nebulosas de emisión + son las nebulosas de absorción (nebulosas oscuras). Estas ni si + quiera están rodeadas de estrellas lo suficientemente potentes ni + cercanas para hacer llegar la luminosidad suficiente para que la + nebulosa pueda reflejarla.</descrip> + <admin type="source">http://www.blogdeastronomia.es/astronomia/formacion-de-estrellas/las-nebulosas</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c31"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Reflection_nebula#/media/File:Reflection.nebula.arp.750pix.jpg">Reflection_Nebula.jpeg</xref> + <note>G-Source: + http://mm04.nasaimages.org/MediaManager/srvr?mediafile=/Size3/NVA2-8-NA/14107/full_tif.jpg&userid=1&username=admin&resolution=3&servertype=JVA&cid=8&iid=NVA2&vcid=NA&usergroup=HUBBLE&profileid=39</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A cloud of interstellar gas and dust that appears + bight because it reflects or scatters starlight.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>reflection nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Just weeks after NASA astronauts repaired the + Hubble Space Telescope in December 1999, the Hubble Heritage Project + snapped this picture of NGC 1999, a reflection nebula in the + constellation Orion. </descrip> + <admin type="source">http://www.nasa.gov/multimedia/imagegallery/image_feature_701.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Nubes de polvo que simplemente reflejan la luz de + una estrella o estrellas cercanas.</descrip> + <admin type="source">http://www.astrored.net/nebulosaweb/types.html</admin> + </descripGrp> + <termSec> + <term>nebulosa de reflexión</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Como el propio nombre implica, esta nebulosa de + reflexión asociada con la estrella Rigel, se asemeja a una vieja + arpía de un cuento de hadas. </descrip> + <admin type="source">http://www.astrofotos.com.es/2008/11/nebulosa-de-la-cabeza-de-bruja.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c32"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Neutron_star#/media/File:PIA18848-PSRB1509-58-ChandraXRay-WiseIR-20141023.jpg">Neutron_Star.jpg</xref> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: http://nrumiano.free.fr/Images/Neutron_star_E.gif</note> + <termSec> + <term>neutron star</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">After its Main Sequence period the star becomes + a red supergiant and may explode as a supernova. It may end as a + neutron star or pulsar, although if its mass is even greater it may + poroduce a black hole.</descrip> + <admin type="source">Moore2003, 173</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: + http://es.wikipedia.org/wiki/Archivo:Estrella_de_Neutrones.jpg</note> + <descripGrp> + <descrip type="definition">Un cuerpo pequeño muy denso que se forma en el + envejecimiento de una estrella pesada y que está formada únicamente por + partículas subatómicas denominadas neutrones.</descrip> + <admin type="source">http://www.astroasa.com.ar/diccionario_astro.htm</admin> + </descripGrp> + <termSec> + <term>estrella de neutrones</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">El Gran Telescopio Canarias (GTC), instalado en + el Observatorio del Roque de los Muchachos (La Palma), ha obtenido + imágenes de una profundidad "sin precedentes" de una estrella de + neutrones del tipo magnetar, de las que se conocen seis, según ha + informado el Instituto de Astrofísica de Canarias (IAC).</descrip> + <admin type="source">http://www.rtve.es/noticias/20100301/imagen-unica-estrella-neutrones-cazada-canarias/321412.shtml</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c33"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The maximum possible mass of a degenerate star, + above which it will be unable to support itself against the inward pull + of its own gravity. </descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <note>For a star with no hydrogen content the limit is 1.44 solar masses, which + is thus the maximum possible for a white dwarf.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>Chandrasekhar limit</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">However, there is a limit, once the mass of the + white dwarf becomes greater than 1.4 time that of the sun )a value + known as the Chandrasekhar limit, after the Indian astronomer who + first worked it out=, the carbon detonates, and in a matter of a few + seconds the white dwarf blows itself to pieces.</descrip> + <admin type="source">Moore2003</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El límite de masa más allá del cual la + degeneración de electrones no es capaz de contrarrestar la fuerza de + gravedad en un remanente estelar, produciéndose un colapso que origina + una estrella de neutrones o un agujero negro. </descrip> + <admin type="source">http://es.wikipedia.org/wiki/L%C3%ADmite_de_Chandrasekhar</admin> + </descripGrp> + <termSec> + <term>límite de Chandrasekhar</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Descubrió una masa (aproximadamente 1.5 veces la + masa del Sol) en la que una estrella fría no podría soportar su + gravedad. Esto es lo que se conoce como el límite de + Chandrasekhar.</descrip> + <admin type="source">http://html.rincondelvago.com/agujeros-negros_5.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c34"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The state of degeneracy attained when the density + of matter is so high that neutrons cannot be packed any more closely + together.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <note>Encountered on in neutron stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>neutron degeneracy</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">When it reaches the threshold of energy + necessary to force the combining of electrons and protons to form + neutrons, the electron degeneracy limit has been passed and the + collapse continues until it is stopped by neutron + degeneracy.</descrip> + <admin type="source">http://hyperphysics.phy-astr.gsu.edu/HBASE/Astro/pulsar.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El estado de degeneración alcanzado cuando la + densidad de materia es tan alta, que los neutrones no pueden juntarse + más.</descrip> + <admin type="source">Oxford2003</admin> + </descripGrp> + <termSec> + <term>degeneración de neutrones</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Es la principal responsable de la resistencia al + colapso gravitacional de las enanas blancas (degeneración de + electrones) y de las estrellas de neutrones (degeneración de + neutrones). </descrip> + <admin type="source">http://www.emiliosilveravazquez.com/glosario.php?letra=d</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c35"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Event_horizon#/media/File:Spacetime_lattice_analogy.svg">Event_Horizon.jpg</xref> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The radius of the event horizon of a black + hole.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>Schwarzschild radius</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The critical radius of a non-rotating black hole + is called the Schwarzschild radius, after the German astronomer who + investermSecated the problem mathematically as long ago as 1916: the + boundary around the collapsed star having this radius is termed the + 'event horizon'.</descrip> + <admin type="source">Moore2003</admin> + </descripGrp> + <note>Related Term: event horizon</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El radio del horizonte de sucesos para un agujero + negro.</descrip> + <admin type="source">http://www.astrocosmo.cl/glosario/glosar-r.htm</admin> + </descripGrp> + <termSec> + <term>radio de Schwarzschild</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Me pareció muy interesante este vídeo del + proyecto Sixty Symbols de la Universidad de Nottingham en el que + explican de forma divulgativa qué es el radio de Schwarzschild. + Básicamente es el radio de un agujero negro.</descrip> + <admin type="source">http://www.microsiervos.com/archivo/ciencia/agujeros-negros-y-el-radio-de-schwarzschild.html</admin> + </descripGrp> + <note>Related Term: horizonte de sucesos, horizonte de eventos</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c36"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Event_horizon#/media/File:Spacetime_lattice_analogy.svg">Event_Horizon.jpg</xref> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The surface of a black hole.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>event horizon</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Narayan and Heyl have calculated that if very + heavy objects do not collapse to a point with an event horizon but + instead have a surface, they would eject as many type 1 bursts as + neutron stars.</descrip> + <admin type="source">http://www.newscientist.com/article/dn2527-astronomers-reach-the-event-horizon.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El superficie de un agujero negro.</descrip> + <admin type="source">Oxford2003</admin> + </descripGrp> + <termSec> + <term>horizonte de sucesos</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">En consecuencia, aquí, cuando nos estamos + refiriendo a una «singularidad», estamos pensando en una masa con + volumen nulo rodeada de una frontera gravitacional llamada + «horizonte de sucesos», de la cual nada puede escapar. </descrip> + <admin type="source">http://www.astrocosmo.cl/h-foton/h-foton-03_08-01.htm</admin> + </descripGrp> + </termSec> + <termSec> + <term>horizonte de eventos</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">InvestermSecadores de la Universidad de St. Andrews + en Escocia, afirman haber encontrado una forma de simular un + horizonte de eventos de un agujero negro – no a través de una nueva + técnica de observación cósmica, ni mediante una supercomputadora de + alta potencia … sino en el laboratorio.</descrip> + <admin type="source">http://www.cienciakanija.com/2008/02/14/horizonte-de-eventos-sintetico-de-un-agujero-negro-creado-en-un-laboratorio-del-reino-unido/</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c37"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Proton%E2%80%93proton_chain_reaction#/media/File:Fusion_in_the_Sun.svg">PP_Chain.jpg</xref> + <note>G-Source: http://en.wikipedia.org/wiki/File:FusionintheSun.svg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <termSec> + <term>proton-proton chain reaction</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">The proton–proton chain reaction is one of + several fusion reactions by which stars convert hydrogen to helium, + the primary alternative being the CNO cycle. The proton–proton chain + dominates in stars the size of the Sun or smaller.</descrip> + <admin type="source">http://www.absoluteastronomy.com/topics/Proton-proton_chain_reaction</admin> + </descripGrp> + </termSec> + <termSec> + <term>PP chain</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">preferredTerm-admn-sts</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">The primary reactions in the main branch of the + PP chain are illustrated in the following figure.</descrip> + <admin type="source">http://csep10.phys.utk.edu/astr162/lect/energy/ppchain.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>proton-proton reaction</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">The gamma rays produced in the proton-proton + reaction take one to 10 million years to work their way out from the + star's core, being scattered numerous times and losing energy as + they go, until they emerge from the surface as rays of light and + heat. Inside the Sun, about 655 million tons of hydrogen are + converted into 650 million tons of helium every second. In stars + heavier than about 2 solar masses, in which the core temperature is + more than about 18 million K, the dominant process in which energy + is produced by the fusion of hydrogen into helium is a different + reaction chain known as the carbon-nitrogen cycle. </descrip> + <admin type="source">http://www.daviddarling.info/encyclopedia/P/proton-proton_chain.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un conjunto de procesos nucleares mediante los + cuales cuatro núcleos de átomos de hidrógeno se combinan para formar uno + de helio, produciendo gran cantidad de energía.</descrip> + <admin type="source">http://www.avizora.com/publicaciones/astronomia/textos/glosario_astronomia_afines_0006.htm</admin> + </descripGrp> + <termSec> + <term>cadena protón-protón</term> + + + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c38"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/CNO_cycle#/media/File:CNO_cycle.png">CNO_Cycle.jpg</xref> + <note>G-Source: http://en.wikipedia.org/wiki/File:CNO_Cycle.svg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <termSec> + <term>carbon-nitrogen cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">The Helium burning process are important 1) + Carbon-Nitrogen cycle at which a carbon-12 nucleus (12C) capture + proton and is converted into 13C, Nitrogen-4 and nitrogen –15. </descrip> + <admin type="source">http://www.sciencenews.org/view/generic/id/44769/title/Supernova_may_be_in_a_new_class</admin> + </descripGrp> + </termSec> + <termSec> + <term>CNO cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">preferredTerm-admn-sts</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">For stars heavier than the sun, theoretical + models show that the CNO (carbon-nitrogen-oxygen) cycle of nuclear + fusion is the dominant source of energy generation.</descrip> + <admin type="source">http://nobelprize.org/nobel_prizes/physics/articles/fusion/sun_cno.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>carbon-nitrogen-oxygen cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">For stars heavier than the sun, theoretical + models show that the CNO (carbon-nitrogen-oxygen) cycle of nuclear + fusion is the dominant source of energy generation.</descrip> + <admin type="source">http://nobelprize.org/nobel_prizes/physics/articles/fusion/sun_cno.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>Bethe-Weizsäcker-cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">Dr. von Weizsäcker is best known in science for + what is sometimes called the Bethe-Weizsäcker cycle, proposed by him + and the physicist Hans Bethe in the late 1930s as the nuclear + reactive process by which energy is generated in stars. </descrip> + <admin type="source">http://www.nytimes.com/2007/05/02/world/europe/02weizsacker.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>carbon cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">deprecatedTerm-admn-sts</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">The main theme of the carbon cycle is the adding + of protons, but after a carbon-12 nucleus fuses with a proton to + form nitrogen-13, one of the protons decays with the emission of a + positron and a neutrino to form carbon -13.</descrip> + <admin type="source">http://hyperphysics.phy-astr.gsu.edu/HBASE/Astro/carbcyc.html</admin> + </descripGrp> + <note>The carbon cycle can also refer to the biogeochemical cycle by which + carbon is exchanged among the biosphere, pedosphere, geosphere, + hydrosphere, and atmosphere of the Earth.</note> + <note>N-Source: http://en.wikipedia.org/wiki/Carbon_cycle</note> + </termSec> + <termSec> + <term>CN cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">We argue that it may be possible to exploit + neutrinos from the CN cycle and p-p chain to determine the + primordial solar core abundances of C and N at an interesting level + of precision.</descrip> + <admin type="source">http://iopscience.iop.org/0004-637X/687/1/678</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <termSec> + <term>ciclo CNO</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">Existen dos formas fundamentales en las que una + estrella fusiona hidrógeno para producir helio: la cadena + protón-protón y el ciclo CNO.</descrip> + <admin type="source">http://eltamiz.com/2007/09/06/la-vida-privada-de-las-estrellas-las-entranas-de-una-estrella/</admin> + </descripGrp> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno-oxígeno</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">deprecatedTerm-admn-sts</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">No se pretende copiar los complicados ciclos de + reacciones que se dan en el interior de las estrellas, como la + cadena protón-protón o el ciclo del carbono-nitrógeno-oxígeno (esta + última más importante en las estrellas más masivas que el Sol). </descrip> + <admin type="source">http://www.zaragoza.es/ciudad/conocimiento/zivis/aplicaciones.htm</admin> + </descripGrp> + </termSec> + <termSec> + <term>ciclo del carbono</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">deprecatedTerm-admn-sts</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">El ciclo del carbono comienza y acaba con un + núcleo de carbono 12 que actúa como catalizador en la producción de + un núcleo de helio a partir de núcleos de hidrógeno; también se + producen neutrinos y rayos gamma. </descrip> + <admin type="source">http://www.astromia.com/glosario/ciclocno.htm</admin> + </descripGrp> + <note>También este término puede referirse a la formación de las moléculas + de carbohidratos, lípidos, proteínas y ácidos nucleicos.</note> + <note>N-Source: http://es.wikipedia.org/wiki/Ciclo_del_carbono</note> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">preferredTerm-admn-sts</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">En las estrellas de gran masa, que queman su + hidrógeno mucho más rápidamente, predomina el ciclo del + carbono-nitrógeno (CN).</descrip> + <admin type="source">http://www.aavbae.net/bol17/evolucion.php</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c39"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A state of matter attained when atomic particles + are packed together as termSechtly as is physically possible, at densities + of several thousand tonnes per cubic metre.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>degeneracy</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Although Eddington raised doubts at the meeting + about the concept of relativistic degeneracy, astronomy has since + found that all white dwarfs for which masses have been measured fall + neatly below the Chandrasekhar limit without exception. Today there + are no doubts about his work on degeneracy. </descrip> + <admin type="source">http://www.tamil.net/people/andrew/subra.htm</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Estado de la materia producido cuando las + partículas atómicas tienen el mayor empaquetamiento físicamente posible, + con densidades de varios miles de toneladas por centímetro cúbico. </descrip> + <admin type="source">http://www.emiliosilveravazquez.com/glosario.php?letra=d</admin> + </descripGrp> + <termSec> + <term>degeneración</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Estas estrellas son aún más densas que las + enanas blancas, y más pequeñas. Se mantienen por un proceso de + "degeneración de neutrones" o "repulsión de neutrones".</descrip> + <admin type="source">http://www.austrinus.com/index.php?option=com_content&view=article&id=157&Itemid=112</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c40"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <termSec> + <term>Oxford2003</term> + + + <note>Author[s]: Ridpath, Ian</note> + <note>Book Title: Astronomía</note> + <note>Publication Place: Spain</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c41"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The state of degeneracy attained when the density + of matter is so high that electrons cannot be packed any closer + together.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <note>Electron degeneracy supports white dwarf stars against further + collapse.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>electron degeneracy</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">When it reaches the threshold of energy + necessary to force the combining of electrons and protons to form + neutrons, the electron degeneracy limit has been passed and the + collapse continues until it is stopped by neutron + degeneracy.</descrip> + <admin type="source">http://hyperphysics.phy-astr.gsu.edu/HBASE/Astro/pulsar.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El estado de degeneración alcanzado cuando la + densidad de materia es tan grande, que los electrones no pueden + empaquetarse más.</descrip> + <admin type="source">Oxford2003</admin> + </descripGrp> + <termSec> + <term>degeneración de electrones</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">Es la principal responsable de la resistencia al + colapso gravitacional de las enanas blancas (degeneración de + electrones) y de las estrellas de neutrones (degeneración de + neutrones). </descrip> + <admin type="source">http://www.emiliosilveravazquez.com/glosario.php?letra=d</admin> + </descripGrp> + </termSec> + <termSec> + <term>degeneración electrónica</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="administrativeStatus">admittedTerm-admn-sts</termNote> + <descripGrp> + <descrip type="context">Las fuerzas gravitatorias actuantes en un cuerpo + celeste masivo pueden comprimir su materia hasta un estado de + degeneración electrónica y no más, ya que el principio de exclusión + impide a dos electrones ocupar el mismo nivel de energía. </descrip> + <admin type="source">http://www.portalplanetasedna.com.ar/estrella2.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c42"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Event_horizon#/media/File:Spacetime_lattice_analogy.svg">Event_Horizon.jpg</xref> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A mathematical point at which certain physical + quantities reach infinite values.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>singularity</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">A singularity means a point where some property + is infinite. For example, at the center of a black hole, according + to classical theory, the density is infinite (because a finite mass + is compressed to a zero volume). Hence it is a singularity. </descrip> + <admin type="source">http://curious.astro.cornell.edu/question.php?number=55</admin> + </descripGrp> + <note>Related Term: black hole, event horizon, Schwarzschild radius</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un punto matemático en el que ciertas cantidades + físicas alcanzan valores infinitos.</descrip> + <admin type="source">Oxford2003</admin> + </descripGrp> + <termSec> + <term>singularidad</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Las singularidades ocurren en el Big Bang, en + los agujeros negros y en el Big Crunch (que podría ser considerado + como una unión de agujeros negros).</descrip> + <admin type="source">http://www.astrocosmo.cl/h-foton/h-foton-03_08-01.htm</admin> + </descripGrp> + <note>Related Term: agujero negro, horizonte de sucesos, radio de + Schwarzschild</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c43"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Solar_mass#/media/File:Rho_Cassiopeiae_Sol_VY_Canis_Majoris.png">Solar_Mass.jpg</xref> + <note>G-Source: http://en.wikipedia.org/wiki/Solar_mass</note> + <note>In this graphic, the M with a subscript is the symbol for a solar mass.</note> + <note>N-Source: Jonathan Tomolonis</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A unit of mass used in stellar and galactic + astronomy, equivalent to the mass of the sun, 1.989 x 10^30 + kg.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>solar mass</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">This page now explores the fate of stars of 8 + solar masses or less.</descrip> + <admin type="source">http://outreach.atnf.csiro.au/education/senior/astrophysics/stellarevolution_deathlow.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una unidad de medida utilizada en astronomía y + astrofísica para medir comparativamente la masa de las estrellas y otros + objetos astronómicos muy masivos como galaxias.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Masa_solar</admin> + </descripGrp> + <termSec> + <term>masa solar</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Para una nube con la masa de nuestro Sol, el + colapso dura unos 10 millones de años, mientras que si su masa fuese + mucho más pequeña, por ejemplo un décimo de la masa solar, este + proceso podría durar hasta 800 millones de años.</descrip> + <admin type="source">http://www.tayabeixo.org/sist_solar/hipotesis/formacion_sistsolar.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c44"> + <descrip type="subjectField">General</descrip> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Triple-alpha_process#/media/File:Triple-Alpha_Process.svg" + >Triple-Alpha_Process.jpg</xref> + <note>G-Source: + http://upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Triple-Alpha_Process.svg/750px-Triple-Alpha_Process.svg.png</note> + <langSec xml:lang="en"> + + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The chain of nuclear reactions by which carbon is + synthesized in the interiors of stars through the fusion of three helium + nuclei(alpha particles).</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>triple-alpha process</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">This small concentration of Be-8 can begin to + undergo reactions with other He-4 nuclei to produce an excited state + of the mass-12 isotope of Carbon. This excited state is unstable, + but a few of these excited Carbon nuclei emit a gamma-ray quickly + enough to become stable before they disintegrate. This extremely + improbable sequence is called the triple-alpha process because the + net effect is to combine 3 alpha particles (that is, 3 He-4 nuclei) + to form a C-12 nucleus. </descrip> + <admin type="source">http://csep10.phys.utk.edu/astr162/lect/energy/triplealph.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El proceso por el cual tres núcleos de helio + (partículas alfa) se transforman en un núcleo de carbono.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Proceso_triple-alfa</admin> + </descripGrp> + <termSec> + <term>proceso triple-alfa</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">También debe tenerse en cuenta una tercera + reacción de gran importancia, denominada proceso triple + alfa.</descrip> + <admin type="source">http://feinstein.com.ar/Composicion.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c45"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Black_dwarf#/media/File:Black_dwarf.jpg">Black_Dwarf.jpg</xref> + <note>G-Source: + http://www.dorlingkindersley-uk.co.uk/static/clipart/uk/dk/sci_space/image_sci_space013.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A degenerate star that has cooled until it is no + longer visible.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>black dwarf</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Banprupt though it is, a white swarf still has a + high surface temperature when it is first formed; up to 100,000 + degrees C in some cases and it continues to radiate. Gradually it + fades, and must end up as a cold, dead black dwarf; but at the + moment no white dwarf with a surface temperature of below 3,000 + degrees C has been found, and it may be that the universe is not yet + old enough for any black dwarfs to have been formed.</descrip> + <admin type="source">Moore2003, 173</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">origination</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una estrella creada cuando una enana blanca se + enfría lo suficiente como para dejar de emitir calor o luz en cantidad + significativa.</descrip> + <admin type="source">http://spaceplace.nasa.gov/sp/kids/spitzer/signs/sign_glossary.shtml</admin> + </descripGrp> + <termSec> + <term>enana negra</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">No se conoce, todavía, la cantidad de Enanas + Negras que pueblan en realidad nuestro Universo. El tiempo estimado + para que una Enana Blanca se enfríe lo suficiente para volverse + Negra, se estima entre diez y cien mil millones de años, y nuestro + Universo no es aún lo bastante viejo, nada más que para que existan + algunas enanas blancas que se han enfriado lo suficiente para + alcanzar la etapa de enanas negras.</descrip> + <admin type="source">http://celestia.albacete.org/celestia/celestia/stars/enana12.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + </body> + <back> + <refObjectSec type="respPerson"> + <refObject id="pe324as3-9615-4d41-a9c8-30c36bffe0e6"> + <item type="fn">Tommy Tomolonis</item> + </refObject> + </refObjectSec> + </back> + </text> + +</tbx> diff --git a/reference-docs/schemas/TBX-Linguist_dialect/DCA/TBX-Linguist_DCA.sch b/reference-docs/schemas/TBX-Linguist_dialect/DCA/TBX-Linguist_DCA.sch new file mode 100644 index 0000000..14bf4f8 --- /dev/null +++ b/reference-docs/schemas/TBX-Linguist_dialect/DCA/TBX-Linguist_DCA.sch @@ -0,0 +1,146 @@ +<?xml version="1.0" encoding="UTF-8"?> +<schema xmlns="http://purl.oclc.org/dsdl/schematron" queryBinding="xslt2" + xmlns:sqf="http://www.schematron-quickfix.com/validator/process"> + <ns uri="urn:iso:std:iso:30042:ed-2" prefix="tbx" /> + <pattern id="coreEnforecement"> + <rule context="tbx:termNote"> +<assert test="parent::tbx:termSec or parent::tbx:termNoteGrp/parent::tbx:termSec">Any termNote is only allowed at the termSec level.</assert> + </rule> + <rule context="tbx:*[@type]"> + <assert test="@type != ''">Data category must be declared. If no permitted data categories are listed in the grammar schema, blank values are also not allowed.</assert> + </rule> + <rule context="*[@target]"> + <assert test="matches(@target,'https?://.+') or @target = //*/@id">ID must be IDREF for internal references or URI following HTTP protocol for external references.</assert> + </rule> + </pattern> + + <pattern id="XLIFF.inlineConstraints"> + <rule context="tbx:sc[following-sibling::tbx:ec]"> + <assert test="@isolated='no' or not(@isolated)">@isolated must be 'no' if <sc/> or <ec/> has its corresponding <sc/>/<ec/> in the same note text and @startRef must be used for <ec></assert> + </rule> + <rule context="tbx:ec[preceding-sibling::tbx:sc]"> + <assert test="@isolated='no' or not(@isolated)">@isolated must be 'no' if <sc/> or <ec/> has its corresponding <sc/>/<ec/> in the same note text and @startRef must be used for <ec></assert> + <assert test="@startRef">@starRef is required for <ec> if it is in the same note text as its corresponding <sc></assert> + <!--<assert test="not(@dir)">@dir only permitted when @isolated is 'yes'.</assert>--><!--@dir IS NOT CURRENTLY USED IN TBX--> + </rule> + <rule context="tbx:sc[not(following-sibling::tbx:ec)]"> + <assert test="@isolated='yes' or not(@isolated)">@isolated must be 'yes' if <sc/> or <ec/> does not have its corresponding <sc/>/<sc/> in the same note text</assert> + </rule> + <rule context="tbx:ec[not(preceding-sibling::tbx:sc)]"> + <assert test="@isolated='yes' or not(@isolated)">@isolated must be 'yes' if <sc/> or <ec/> does not have its corresponding <sc/>/<sc/> in the same note text</assert> + <assert test="@id">@id is REQUIRED when @isolated is or should be 'yes'.</assert> + </rule> + <rule context="tbx:ec[@isolated='yes']"> + <assert test="@id != ''">ID is required if @isolated is 'yes'.</assert> + </rule> + </pattern> + + <pattern id="dialectEnforcement"> + <rule context="tbx:tbx"> +<assert test="attribute::type='TBX-Linguist'">The name of this dialect should be TBX-Linguist</assert> +<assert test="attribute::style='dca'">The style of this dialect should be declared as 'dca'</assert> + </rule> + <rule context="*[not(namespace-uri() = 'urn:iso:std:iso:30042:ed-2')]"> + <assert test="false()">DCT style elements are not permitted in DCA style TBX.</assert> + </rule> + </pattern> + + <!-- Min Module Rules --> + <pattern id="module.min.admin"> + <rule context="tbx:admin[@type='customerSubset']"> + <assert test="parent::tbx:conceptEntry or parent::adminGrp/parent::tbx:conceptEntry or + parent::tbx:termSec or parent::tbx:adminGrp/parent::tbx:termSec">Customer Subset may only appear at the conceptEntry or termSec levels</assert> + </rule> + </pattern> + <pattern id="module.min.descrip"> + <rule context="tbx:descrip[@type='subjectField']" > +<assert test="parent::tbx:conceptEntry or parent::tbx:descripGrp/parent::tbx:conceptEntry">Subject Field can only appear at conceptEntry level.</assert> + </rule> + </pattern> + <pattern id="module.min.termNote"> + <rule context="tbx:termNote[@type='administrativeStatus']"> + <assert test=".='admittedTerm-admn-sts' or .='deprecatedTerm-admn-sts' or .='supersededTerm-admn-sts' or .='preferredTerm-admn-sts'">The termType must be either 'admittedTerm-admn-sts', 'deprecatedTerm-admn-sts', 'supersededTerm-admn-sts', or 'preferredTerm-admn-sts'</assert> + </rule> + <rule context="tbx:termNote[@type='partOfSpeech']"> + <assert test=".='adjective' or .='noun' or .='other' or .='verb' or .='adverb'">Permitted values of /partOfSpeech/ are 'noun', 'other', 'verb', 'adverb', or 'adjective'</assert> + </rule> + </pattern> + + <!-- Basic Module Rules --> + <pattern id="module.basic.admin"> + <rule context="tbx:admin[@type='projectSubset']"> + <assert test="parent::tbx:conceptEntry or parent::tbx:termSec or parent::adminGrp/(parent::tbx:conceptEntry or + parent::tbx:termSec)">Project may only appear at the conceptEntry or termSec levels</assert> + </rule> + <rule context="tbx:admin[@type='source']"> + <assert test="parent::tbx:conceptEntry or parent::tbx:langSec or parent::tbx:termSec or + parent::tbx:descripGrp/(parent::tbx:conceptEntry or parent::tbx:langSec or parent::tbx:termSec)"></assert> + </rule> + </pattern> + <pattern id="module.basic.descrip"> + <rule context="tbx:descrip[@type='context']"> + <assert test="parent::tbx:termSec or parent::tbx:descripGrp/parent::tbx:termSec">Context appears at the termSec level</assert> + </rule> + <rule context="tbx:descrip[@type='definition']"> + <assert test="parent::tbx:conceptEntry or parent::tbx:langSec or + parent::tbx:descripGrp/(parent::tbx:conceptEntry or parent::tbx:langSec)"> + Definition may appear at the conceptEntry or langSec levels. + </assert> + </rule> + </pattern> + <pattern id="module.basic.termNote"> + <rule context="tbx:termNote[@type='grammaticalGender']"> + <assert test=".='masculine' or .='feminine' or .='neuter' or .='other'">Permitted values of Gender are 'masculine', 'feminine', 'neuter', or 'other'</assert> + </rule> + <rule context="tbx:termNote[@type='termLocation']"> + <assert test=".='checkBox' or .='comboBox' or .='comboBoxElement' or .='dialogBox' or .='groupBox' or .='informativeMessage' or .='interactiveMessage' or .='menuItem' or + .='progressBar' or .='pushButton' or .='radioButton' or .='slider' or .='spinBox' or .='tab' or .='tableText' or .='textBox' or .='toolTip' or .='user-definedType'"> + Permitted values are: checkBox, comboBox, comboBoxElement, dialogBox, groupBox, informativeMessage, interactiveMessage, menuItem, progressBar, pushButton, radioButton, slider, spinBox, tab, tableText, textBox, toolTip, user-definedType + </assert> + </rule> + <rule context="tbx:termNote[@type='termType']"> + <assert test=".='fullForm' or .='acronym' or .='abbreviation' or .='shortForm' or .='variant' or .='phrase'">Permitted values of Term Type are 'fullForm', 'acronym', 'abbreviation', 'shortForm', 'variant', or 'phrase'</assert> + </rule> + </pattern> + <pattern id="module.basic.transac"> + <rule context="tbx:transac[@type='transactionType']"> + <assert test=".='origination' or .='modification'">Transaction type may be either 'origination' or 'modification'.</assert> + </rule> + </pattern> + <pattern id="module.basic.ref"> + <rule context="tbx:ref[@type='crossReference']"> + <assert test="parent::tbx:conceptEntry or parent::tbx:termSec or parent::tbx:*[contains(.,Grp)]/(parent::tbx:conceptEntry or parent::tbx:termSec)">Cross Reference must only be found at the conceptEntry or termSec levels.</assert> + </rule> + </pattern> + <pattern id="module.basic.xref"> + <rule context="tbx:xref[@type='externalCrossReference']"> + <assert test="parent::tbx:conceptEntry or parent::tbx:termSec or parent::tbx:*[contains(.,Grp)]/(parent::tbx:conceptEntry or parent::tbx:termSec)">External Cross Reference must only be found at the conceptEntry or termSec levels.</assert> + </rule> + <rule context="tbx:xref[@type='xGraphic']"> + <assert test="parent::tbx:conceptEntry or parent::tbx:langSec">Image must only be found at the conceptEntry or langSec levels.</assert> + </rule> + </pattern> + + <!-- Linguist Module Rules --> + <pattern id="module.linguist.admin"> + <rule context="tbx:admin[@type='reading']"> + <assert test="parent::tbx:termSec or parent::tbx:adminGrp/parent::tbx:termSec">Reading must be at the term level.</assert> + </rule> + </pattern> + + <pattern id="module.linguist.adminNote"> + <rule context="tbx:adminNote[@type='readingNote']"> + <assert test="parent::tbx:adminGrp/parent::tbx:termSec">readingNote may only be found at the termSec level inside an adminGrp.</assert> + </rule> + </pattern> + + <pattern id="module.linguist.termNote"> + <rule context="tbx:termNote[@type='grammaticalNumber']"> + <assert test=".='singular' or .='plural' or .='dual' or .='mass' or .='otherNumber'">Permitted values of grammaticalNumber are: singular, plural, dual, mass, or otherNumber.</assert> + </rule> + <rule context="tbx:termNote[@type='register']"> + <assert test=".='colloquialRegister' or .='neutralRegister' or .='technicalRegister' or .='in-houseRegister' or .='bench-levelRegister' or .='slangRegister' or .='vulgarRegister'">Permitted values of register are: + colloquialRegister, neutralRegister, technicalRegister, in-houseRegister, bench-levelRegister, slangRegister, or vulgarRegister</assert> + </rule> + </pattern> +</schema> \ No newline at end of file diff --git a/reference-docs/schemas/TBX-Linguist_dialect/DCA/TBXcoreStructV03_TBX-Linguist_integrated.rng b/reference-docs/schemas/TBX-Linguist_dialect/DCA/TBXcoreStructV03_TBX-Linguist_integrated.rng new file mode 100644 index 0000000..f386e1b --- /dev/null +++ b/reference-docs/schemas/TBX-Linguist_dialect/DCA/TBXcoreStructV03_TBX-Linguist_integrated.rng @@ -0,0 +1,1198 @@ +<?xml version="1.0" encoding="utf-8"?> +<grammar xmlns="http://relaxng.org/ns/structure/1.0" + datatypeLibrary="http://www.w3.org/2001/XMLSchema-datatypes" ns="urn:iso:std:iso:30042:ed-2"> + <define name="entity.basicText"> + <zeroOrMore> + <choice> + <text/> + <ref name="hi"/> + </choice> + </zeroOrMore> + </define> + <define name="entity.noteText"> + <zeroOrMore> + <choice> + <text/> + <ref name="hi"/> + <ref name="foreign"/> + <ref name="sc"/> + <ref name="ec"/> + <ref name="ph"/> + </choice> + </zeroOrMore> + </define> + <define name="entity.auxInfo"> + <choice> + <zeroOrMore> + <choice> + <ref name="descrip"/> + <ref name="descripGrp"/> + <ref name="admin"/> + <ref name="adminGrp"/> + <ref name="transacGrp"/> + <ref name="note"/> + <ref name="ref"/> + <ref name="xref"/> + </choice> + </zeroOrMore> + <zeroOrMore> + <choice> + <ref name="note"/> + <ref name="adminGrp"/> + <ref name="descripGrp"/> + <ref name="transacGrp"/> + <ref name="DCTnamespaceElements"/> + </choice> + </zeroOrMore> + </choice> + </define> + <define name="entity.noteLinkInfo"> + <choice> + <zeroOrMore> + <choice> + <ref name="admin"/> + <ref name="adminGrp"/> + <ref name="transacGrp"/> + <ref name="note"/> + <ref name="ref"/> + <ref name="xref"/> + </choice> + </zeroOrMore> + <zeroOrMore> + <choice> + <ref name="adminGrp"/> + <ref name="transacGrp"/> + <ref name="note"/> + <ref name="DCTnamespaceElements"/> + </choice> + </zeroOrMore> + </choice> + </define> + <define name="idlang.attributes"> + <ref name="id.attributes"/> + <ref name="lang.attributes"/> + </define> + <define name="idtype.attributes"> + <ref name="id.attributes"/> + <ref name="idtype.attribute.type"/> + </define> + <define name="idtype.attribute.type"> + <optional> + <attribute name="type"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the type of the meta data-category.</a:documentation> + <text/> + </attribute> + </optional> + </define> + <define name="id.attributes"> + <optional> + <ref name="id.attribute.id"/> + </optional> + </define> + <define name="id.attribute.id"> + <attribute name="id"> + <data type="ID"/> + </attribute> + </define> + <define name="target-IDREF.attributes"> + <ref name="target-IDREF.attribute.target"/> + </define> + <define name="target-IDREF.attribute.target"> + <optional> + <attribute name="target"> + <data type="IDREF"/> + </attribute> + </optional> + </define> + <define name="lang.attributes"> + <ref name="lang.attribute.xmllang"/> + </define> + <define name="lang.attribute.xmllang"> + <optional> + <attribute name="xml:lang"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the language of the element content. The allowed values are found in IETF RFC 4646 or + its successor. This attribute is optional for elements that use this attribute class. + For a description, see the information at the tbx element.</a:documentation> + <data type="language"/> + </attribute> + </optional> + </define> + <define name="IDLangTgtDtyp.attributes"> + <ref name="lang.attributes"/> + <ref name="id.attributes"/> + <ref name="target-IDREF.attributes"/> + <ref name="IDLangTgtDtyp.attribute.datatype"/> + </define> + <define name="IDLangTgtDtyp.attribute.datatype"> + <optional> + <attribute name="datatype"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">The data + type of plainText, or what is known as PCDATA.</a:documentation> + <text/> + </attribute> + </optional> + </define> + <define name="dispEquivSubType.attributes"> + <optional> + <attribute name="disp"> + <text/> + </attribute> + <attribute name="equiv"> + <text/> + </attribute> + <choice> + <group> + <attribute name="subType"> + <data type="string"> + <param name="pattern">[^\s:]+:[^\s:]+</param> + </data> + </attribute> + <ref name="XLIFFinlineType.attribute"/> + </group> + <ref name="XLIFFinlineType.attribute"/> + </choice> + </optional> + </define> + <define name="XLIFFisolated.attribute"> + <optional> + <attribute name="isolated"> + <choice> + <value>yes</value> + <value>no</value> + </choice> + </attribute> + </optional> + </define> + <define name="XLIFFinlineType.attribute"> + <attribute name="type"> + <choice> + <value>fmt</value> + <value>ui</value> + <value>quote</value> + <value>link</value> + <value>image</value> + <value>other</value> + </choice> + </attribute> + </define> + <define name="hi"> + <element name="hi"> + + <ref name="hi.content"/> + <ref name="hi.localattributes"/> + </element> + </define> + <define name="hi.content"> + <text/> + </define> + <define name="hi.localattributes"> + <ref name="target-IDREF.attributes"/> + <ref name="lang.attributes"/> + <optional> + <attribute name="type"> + + <choice> + <value>entailedTerm</value> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0"> + (entailedTerm) A term, found in the content of a text element such as , that is + defined in another terminological entry in the same terminological + collection.</a:documentation> + <value>hotkey</value> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0"> + (hotkey) A key or a combination of keys on a computer keyboard that, when pressed + at one time, performs a task (such as starting an application) as an alternative + to using a mouse or other input device. Hotkeys are supported by many operating + systems and applications (the hotkey is indicated by an ampersand in the term and + by an underscore in the visual display). This type of hi element allows a hotkey + to be identified as such in a text field such as a context sentence. To identify a + hotkey for the head term of an entry, use the lionHotkey value of the type + attribute on a termNote.</a:documentation> + <value>italics</value> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0"> + (italics) Indicates that the content enclosed in the hi element must be rendered + in italics. </a:documentation> + <value>bold</value> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0"> + (bold) Indicates that the content enclosed in the hi element must be rendered in + boldface. </a:documentation> + <value>superscript</value> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0"> + (superscript) Indicates that the content enclosed in the hi element must be + rendered in superscript. </a:documentation> + <value>subscript</value> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0"> + (subscript) Indicates that the content enclosed in the hi element must be rendered + in subscript.</a:documentation> + <value>math</value> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0"> + (math) Indicates that the content enclosed in the hi element is mathematical in + nature.</a:documentation> + </choice> + </attribute> + </optional> + </define> + <define name="foreign"> + <element name="foreign"> + + <ref name="foreign.content"/> + <ref name="foreign.localattributes"/> + </element> + </define> + <define name="foreign.content"> + <ref name="entity.noteText"/> + </define> + <define name="foreign.localattributes"> + <ref name="idlang.attributes"/> + </define> + <define name="sc"> + <element name="sc"> + + <ref name="sc.content"/> + <ref name="sc.localattributes"/> + </element> + </define> + <define name="sc.content"> + <empty/> + </define> + <define name="sc.localattributes"> + <attribute name="id"> + <data type="ID"/> + </attribute> + <optional> + <ref name="dispEquivSubType.attributes"/> + <ref name="target-IDREF.attributes"/> + <ref name="XLIFFisolated.attribute"/> + </optional> + </define> + <define name="ec"> + <element name="ec"> + + <ref name="ec.content"/> + <ref name="ec.localattributes"/> + </element> + </define> + <define name="ec.content"> + <empty/> + </define> + <define name="ec.localattributes"> + <optional> + <attribute name="id"> + <data type="ID"/> + </attribute> + <attribute name="startRef"> + <data type="IDREF"/> + </attribute> + <ref name="dispEquivSubType.attributes"/> + <ref name="XLIFFisolated.attribute"/> + <ref name="target-IDREF.attributes"/> + </optional> + </define> + <define name="ph"> + <element name="ph"> + <ref name="ph.content"/> + <ref name="ph.localattributes"/> + </element> + </define> + <define name="ph.content"> + <empty/> + </define> + <define name="ph.localattributes"> + <optional> + <attribute name="id"> + <data type="ID"/> + </attribute> + <ref name="dispEquivSubType.attributes"/> + </optional> + </define> + <define name="admin"> + <element name="admin"> + + <ref name="admin.content"/> + <ref name="admin.localattributes"/> + </element> + </define> + <define name="admin.content"> + <ref name="entity.noteText"/> + </define> + <define name="admin.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the data-category type of the admin element, such as originatingDatabase or + entrySource.</a:documentation> + + <ref name="admin.types"/> + + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="adminGrp"> + <element name="adminGrp"> + + <ref name="adminGrp.content"/> + <ref name="adminGrp.localattributes"/> + </element> + </define> + <define name="adminGrp.content"> + <choice> + <group> + <ref name="admin"/> + <zeroOrMore> + <choice> + <ref name="adminNote"/> + <ref name="note"/> + <ref name="ref"/> + <ref name="xref"/> + </choice> + </zeroOrMore> + </group> + <group> + <ref name="DCTnamespaceElements"/> + <zeroOrMore> + <choice> + <ref name="note"/> + <ref name="DCTnamespaceElements"/> + </choice> + </zeroOrMore> + </group> + </choice> + </define> + <define name="adminGrp.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="adminNote"> + <element name="adminNote"> + + <ref name="adminNote.content"/> + <ref name="adminNote.localattributes"/> + </element> + </define> + <define name="adminNote.content"> + <text/> + </define> + <define name="adminNote.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + + + <ref name="adminNote.types"/> + + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="date"> + <element name="date"> + + <ref name="date.content"/> + <ref name="date.localattributes"/> + </element> + </define> + <define name="date.content"> + <data type="date"/> + </define> + <define name="date.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="descrip"> + <element name="descrip"> + + <ref name="descrip.content"/> + <ref name="descrip.localattributes"/> + </element> + </define> + <define name="descrip.content"> + <ref name="entity.noteText"/> + </define> + <define name="descrip.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the data-category type of the descrip element, such as definition or + associated-concept.</a:documentation> + + <ref name="descrip.types"/> + + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="descripGrp"> + <element name="descripGrp"> + + <ref name="descripGrp.content"/> + <ref name="descripGrp.localattributes"/> + </element> + </define> + <define name="descripGrp.content"> + <choice> + <group> + <ref name="descrip"/> + <zeroOrMore> + <choice> + <ref name="descripNote"/> + <ref name="admin"/> + <ref name="adminGrp"/> + <ref name="transacGrp"/> + <ref name="note"/> + <ref name="ref"/> + <ref name="xref"/> + </choice> + </zeroOrMore> + </group> + <group> + <ref name="DCTnamespaceElements"/> + <zeroOrMore> + <choice> + <ref name="note"/> + <ref name="adminGrp"/> + <ref name="transacGrp"/> + <ref name="DCTnamespaceElements"/> + </choice> + </zeroOrMore> + </group> + </choice> + </define> + <define name="descripGrp.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="descripNote"> + <element name="descripNote"> + + <ref name="descripNote.content"/> + <ref name="descripNote.localattributes"/> + </element> + </define> + <define name="descripNote.content"> + <text/> + </define> + <define name="descripNote.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the data-category type of the descripNote element, such as + contextType.</a:documentation> + + <ref name="descripNote.types"/> + + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="langSec"> + <element name="langSec"> + + <ref name="langSec.content"/> + <ref name="langSec.localattributes"/> + </element> + </define> + <define name="langSec.content"> + <ref name="entity.auxInfo"/> + <oneOrMore> + <choice> + <ref name="termSec"/> + </choice> + </oneOrMore> + </define> + <define name="langSec.localattributes"> + <attribute name="xml:lang"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the language of the language section. This attribute is required for the langSec + element. See also the description on the tbx element.</a:documentation> + <text/> + </attribute> + </define> + <define name="note"> + <element name="note"> + + <ref name="note.content"/> + <ref name="note.localattributes"/> + </element> + </define> + <define name="note.content"> + <ref name="entity.noteText"/> + </define> + <define name="note.localattributes"> + <ref name="idlang.attributes"/> + </define> + <define name="ref"> + <element name="ref"> + + <ref name="ref.content"/> + <ref name="ref.localattributes"/> + </element> + </define> + <define name="ref.content"> + <text/> + </define> + <define name="ref.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + + + <ref name="ref.types"/> + + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="term"> + <element name="term"> + <ref name="term.content"/> + <ref name="term.localattributes"/> + </element> + </define> + <define name="term.content"> + <ref name="entity.basicText"/> + </define> + <define name="term.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="conceptEntry"> + <element name="conceptEntry"> + + <ref name="conceptEntry.content"/> + <ref name="conceptEntry.localattributes"/> + </element> + </define> + <define name="conceptEntry.content"> + <ref name="entity.auxInfo"/> + <oneOrMore> + <ref name="langSec"/> + </oneOrMore> + </define> + <define name="conceptEntry.localattributes"> + <ref name="id.attribute.id"/> + </define> + <define name="termNote"> + <element name="termNote"> + <ref name="termNote.content"/> + <ref name="termNote.localattributes"/> + </element> + </define> + <define name="termNote.content"> + <ref name="entity.noteText"/> + </define> + <define name="termNote.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the data-category type of the termNote, such as partOfSpeech or + termType.</a:documentation> + <ref name="termNote.types"/> + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="termNoteGrp"> + <element name="termNoteGrp"> + <ref name="termNoteGrp.content"/> + <ref name="termNoteGrp.localattributes"/> + </element> + </define> + <define name="termNoteGrp.content"> + <choice> + <ref name="termNote"/> + <ref name="DCTnamespaceElements"/> + </choice> + <ref name="entity.noteLinkInfo"/> + </define> + <define name="termNoteGrp.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="termSec"> + <element name="termSec"> + <ref name="termSec.content"/> + <ref name="termSec.localattributes"/> + </element> + </define> + <define name="termSec.content"> + <ref name="term"/> + <choice> + <zeroOrMore> + <choice> + <ref name="termNote"/> + <ref name="termNoteGrp"/> + </choice> + </zeroOrMore> + <zeroOrMore> + <ref name="DCTnamespaceElements"/> + </zeroOrMore> + </choice> + <ref name="entity.auxInfo"/> + </define> + <define name="termSec.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="transac"> + <element name="transac"> + <ref name="transac.content"/> + <ref name="transac.localattributes"/> + </element> + </define> + <define name="transac.content"> + <text/> + </define> + <define name="transac.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">The + attribute value transactionType ensures that the content of the transac element will be + a transaction type.</a:documentation> + <ref name="transac.types"/> + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="transacGrp"> + <element name="transacGrp"> + <ref name="transacGrp.content"/> + <ref name="transacGrp.localattributes"/> + </element> + </define> + <define name="transacGrp.content"> + <choice> + <group> + <ref name="transac"/> + <zeroOrMore> + <choice> + <ref name="transacNote"/> + <ref name="date"/> + <ref name="note"/> + <ref name="ref"/> + <ref name="xref"/> + </choice> + </zeroOrMore> + </group> + <group> + <ref name="DCTnamespaceElements"/> + <zeroOrMore> + <choice> + <ref name="date"/> + <ref name="note"/> + <ref name="DCTnamespaceElements"/> + </choice> + </zeroOrMore> + </group> + </choice> + </define> + <define name="transacGrp.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="transacNote"> + <element name="transacNote"> + + <ref name="transacNote.content"/> + <ref name="transacNote.localattributes"/> + </element> + </define> + <define name="transacNote.content"> + <text/> + </define> + <define name="transacNote.localattributes"> + <ref name="IDLangTgtDtyp.attributes"/> + <attribute name="type"> + <ref name="transacNote.types"/> + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="xref"> + <element name="xref"> + <ref name="xref.content"/> + <ref name="xref.localattributes"/> + </element> + </define> + <define name="xref.content"> + <text/> + </define> + <define name="xref.localattributes"> + <ref name="id.attributes"/> + <attribute name="target"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">The URI of + the external object.</a:documentation> + <data type="anyURI"> + <param name="pattern">https?://.+</param> + </data> + </attribute> + <attribute name="type"> + <ref name="xref.types"/> + </attribute> + <ref name="dca.attributes"/> + </define> + <define name="tbx"> + <element name="tbx"> + <ref name="tbx.content"/> + <ref name="tbx.localattributes"/> + </element> + </define> + <define name="tbx.content"> + <ref name="tbxHeader"/> + <ref name="text"/> + </define> + <define name="tbx.localattributes"> + <attribute name="style"> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> Indicates + whether the file adheres to Data Category as Tag or Data Category as Attribute, DCT or + DCA, style. </documentation> + <choice> + <value>dca</value> + <value>dct</value> + </choice> + </attribute> + <attribute name="xml:lang"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the default language of the entire tbx element content. The allowed values of the + xml:lang attribute are found in IETF RFC 4646 or its successor, as indicated in IETF BCP + 47. This attribute is required for the tbx element.</a:documentation> + <text/> + </attribute> + <attribute name="type"> + <a:documentation xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0">Indicates + the type of tbx document. If the type attribute value TBX is used, then the TBX document + instance shall adhere to the default XCS file. If the TBX document instance adheres to + another XCS file, then the type attribute value can consist of TBX- plus another word + associated with the XCS file, such as 'TBX-Basic'.</a:documentation> + <data type="string"> + <param name="pattern">TBX-.+</param> + </data> + </attribute> + </define> + <define name="tbxHeader"> + <element name="tbxHeader"> + <ref name="tbxHeader.content"/> + <ref name="tbxHeader.localattributes"/> + </element> + </define> + <define name="tbxHeader.content"> + <ref name="fileDesc"/> + <optional> + <ref name="encodingDesc"/> + </optional> + <optional> + <ref name="revisionDesc"/> + </optional> + </define> + <define name="tbxHeader.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="p"> + <element name="p"> + + <ref name="p.content"/> + <ref name="p.localattributes"/> + </element> + </define> + <define name="p.content"> + <ref name="entity.noteText"/> + </define> + <define name="p.localattributes"> + <ref name="idlang.attributes"/> + <optional> + <attribute name="type"> + <text/> + </attribute> + </optional> + </define> + <define name="fileDesc"> + <element name="fileDesc"> + + <ref name="fileDesc.content"/> + <ref name="fileDesc.localattributes"/> + </element> + </define> + <define name="fileDesc.content"> + <optional> + <ref name="titleStmt"/> + </optional> + <optional> + <ref name="publicationStmt"/> + </optional> + <oneOrMore> + <ref name="sourceDesc"/> + </oneOrMore> + </define> + <define name="fileDesc.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="titleStmt"> + <element name="titleStmt"> + + <ref name="titleStmt.content"/> + <ref name="titleStmt.localattributes"/> + </element> + </define> + <define name="titleStmt.content"> + <ref name="title"/> + <zeroOrMore> + <ref name="note"/> + </zeroOrMore> + </define> + <define name="titleStmt.localattributes"> + <ref name="idlang.attributes"/> + </define> + <define name="title"> + <element name="title"> + + <ref name="title.content"/> + <ref name="title.localattributes"/> + </element> + </define> + <define name="title.content"> + <text/> + </define> + <define name="title.localattributes"> + <ref name="idlang.attributes"/> + </define> + <define name="publicationStmt"> + <element name="publicationStmt"> + + <ref name="publicationStmt.content"/> + <ref name="publicationStmt.localattributes"/> + </element> + </define> + <define name="publicationStmt.content"> + <oneOrMore> + <ref name="p"/> + </oneOrMore> + </define> + <define name="publicationStmt.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="sourceDesc"> + <element name="sourceDesc"> + <ref name="sourceDesc.content"/> + <ref name="sourceDesc.localattributes"/> + </element> + </define> + <define name="sourceDesc.content"> + <oneOrMore> + <ref name="p"/> + </oneOrMore> + </define> + <define name="sourceDesc.localattributes"> + <ref name="idlang.attributes"/> + </define> + <define name="encodingDesc"> + <element name="encodingDesc"> + + <ref name="encodingDesc.content"/> + <ref name="encodingDesc.localattributes"/> + </element> + </define> + <define name="encodingDesc.content"> + <oneOrMore> + <ref name="p"/> + </oneOrMore> + </define> + <define name="encodingDesc.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="revisionDesc"> + <element name="revisionDesc"> + + <ref name="revisionDesc.content"/> + <ref name="revisionDesc.localattributes"/> + </element> + </define> + <define name="revisionDesc.content"> + <oneOrMore> + <ref name="change"/> + </oneOrMore> + </define> + <define name="revisionDesc.localattributes"> + <ref name="idlang.attributes"/> + </define> + <define name="change"> + <element name="change"> + + <ref name="change.content"/> + <ref name="change.localattributes"/> + </element> + </define> + <define name="change.content"> + <oneOrMore> + <ref name="p"/> + </oneOrMore> + </define> + <define name="change.localattributes"> + <ref name="idlang.attributes"/> + </define> + <define name="text"> + <element name="text"> + + <ref name="text.content"/> + <ref name="text.localattributes"/> + </element> + </define> + <define name="text.content"> + <ref name="body"/> + <optional> + <ref name="back"/> + </optional> + </define> + <define name="text.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="body"> + <element name="body"> + + <ref name="body.content"/> + <ref name="body.localattributes"/> + </element> + </define> + <define name="body.content"> + <oneOrMore> + <ref name="conceptEntry"/> + </oneOrMore> + </define> + <define name="body.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="back"> + <element name="back"> + + <ref name="back.content"/> + <ref name="back.localattributes"/> + </element> + </define> + <define name="back.content"> + <zeroOrMore> + <ref name="refObjectSec"/> + </zeroOrMore> + </define> + <define name="back.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="refObjectSec"> + <element name="refObjectSec"> + + <ref name="refObjectSec.content"/> + <ref name="refObjectSec.localattributes"/> + </element> + </define> + <define name="refObjectSec.content"> + <oneOrMore> + <ref name="refObject"/> + </oneOrMore> + </define> + <define name="refObjectSec.localattributes"> + <ref name="id.attributes"/> + <attribute name="type"> + <text/> + </attribute> + </define> + <define name="refObject"> + <element name="refObject"> + <ref name="refObject.content"/> + <ref name="refObject.localattributes"/> + </element> + </define> + <define name="refObject.content"> + <oneOrMore> + <choice> + <ref name="itemSet"/> + <ref name="itemGrp"/> + <ref name="item"/> + </choice> + </oneOrMore> + </define> + <define name="refObject.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="item"> + <element name="item"> + + <ref name="item.content"/> + <ref name="item.localattributes"/> + </element> + </define> + <define name="item.content"> + <ref name="entity.noteText"/> + </define> + <define name="item.localattributes"> + <ref name="idtype.attributes"/> + </define> + <define name="itemGrp"> + <element name="itemGrp"> + + <ref name="itemGrp.content"/> + <ref name="itemGrp.localattributes"/> + </element> + </define> + <define name="itemGrp.content"> + <ref name="item"/> + <ref name="entity.noteLinkInfo"/> + </define> + <define name="itemGrp.localattributes"> + <ref name="id.attributes"/> + </define> + <define name="itemSet"> + <element name="itemSet"> + + <ref name="itemSet.content"/> + <ref name="itemSet.localattributes"/> + </element> + </define> + <define name="itemSet.content"> + <oneOrMore> + <choice> + <ref name="item"/> + <ref name="itemGrp"/> + </choice> + </oneOrMore> + </define> + <define name="itemSet.localattributes"> + <ref name="idtype.attributes"/> + </define> + + + + <!-- DCA specific module attribute --> + <define name="dca.attributes"> + <optional> + <attribute name="module"> + <text/> + </attribute> + </optional> + </define> + + <!-- Extension Points for DCT --> + <define name="DCTnamespaceElements"> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> This is an + extension point for TBX data categories which are brought in from another namespace to form + a dialect. </documentation> + <element> + <anyName> + <except> + <nsName ns="urn:iso:std:iso:30042:ed-2"/> + </except> + </anyName> + <zeroOrMore> + <choice> + <attribute> + <anyName> + <except> + <nsName ns="urn:iso:std:iso:30042:ed-2"/> + </except> + </anyName> + </attribute> + <text/> + <ref name="DCTnamespaceElements"/> + </choice> + </zeroOrMore> + </element> + </define> + + <!-- Extension Points for DCA type values. If co-constraint validation is required, such constraints must be supplied via a Schematron file --> + <define name="admin.types"> + + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in DCA, replace <text/> with the allowed + values of the "type" attribute.</p> + </documentation> + <value>customerSubset</value> + <value>projectSubset</value> + <value>reading</value> + <value>source</value> + </choice> + + </define> + <define name="adminNote.types"> + + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in DCA, replace <text/> with the allowed + values of the "type" attribute.</p> + </documentation> + <value>readingNote</value> + </choice> + </define> + + <define name="descrip.types"> + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in DCA, replace <text/> with the allowed + values of the "type" attribute.</p> + </documentation> + <value>context</value> + <value>definition</value> + <value>subjectField</value> + </choice> + </define> + + <define name="descripNote.types"> + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in DCA, replace <text/> with the allowed + values of the "type" attribute.</p> + </documentation> + <empty/> + </choice> + + </define> + <define name="ref.types"> + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in DCA, replace <text/> with the allowed + values of the "type" attribute.</p> + </documentation> + <value>crossReference</value> + </choice> + + </define> + <define name="transac.types"> + + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in DCA, replace <text/> with the allowed + values of the "type" attribute.</p> + </documentation> + <value>transactionType</value> + </choice> + + </define> + <define name="transacNote.types"> + + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in DCA, replace <text/> with the allowed + values of the "type" attribute.</p> + </documentation> + <value>responsibility</value> + </choice> + + </define> + <define name="xref.types"> + + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in DCA, replace <text/> with the allowed + values of the "type" attribute.</p> + </documentation> + <value>externalCrossReference</value> + <value>xGraphic</value> + </choice> + + </define> + + <define name="termNote.types"> + + <choice> + <documentation xmlns="http://relaxng.org/ns/compatibility/annotations/1.0"> + <p>For an integrated schema for use in DCA, replace <text/> with the allowed + values of the "type" attribute.</p> + </documentation> + <value>administrativeStatus</value> + <value>grammaticalGender</value> + <value>geographicalUsage</value> + <value>grammaticalNumber</value> + <value>partOfSpeech</value> + <value>register</value> + <value>termLocation</value> + <value>termType</value> + <value>transferComment</value> + </choice> + + </define> + + <start> + <ref name="tbx"/> + </start> +</grammar> diff --git a/reference-docs/schemas/TBX-Linguist_dialect/DCT/Example_Astronomy_DCT_VALID.tbx b/reference-docs/schemas/TBX-Linguist_dialect/DCT/Example_Astronomy_DCT_VALID.tbx new file mode 100644 index 0000000..13c4c99 --- /dev/null +++ b/reference-docs/schemas/TBX-Linguist_dialect/DCT/Example_Astronomy_DCT_VALID.tbx @@ -0,0 +1,4019 @@ +<?xml version="1.0" encoding="utf-8"?> +<?xml-model href="https://raw.githubusercontent.com/LTAC-Global/TBX-Linguist_dialect/master/DCT/TBX-Linguist.nvdl" type="application/xml" schematypens="http://purl.oclc.org/dsdl/nvdl/ns/structure/1.0"?> +<tbx type="TBX-Linguist" style="dct" xml:lang="en" xmlns="urn:iso:std:iso:30042:ed-2" xmlns:min="http://www.tbxinfo.net/ns/min" xmlns:basic="http://www.tbxinfo.net/ns/basic" xmlns:ling="http://www.tbxinfo.net/ns/linguist"> + <tbxHeader> + <fileDesc> + <sourceDesc> + <p>TBX file, created via MultiTerm Export</p> + </sourceDesc> + </fileDesc> + </tbxHeader> + + <text> + <body> + <conceptEntry id="c1"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Galaxy_cluster#/media/File:Galaxy_cluster_IDCS_J1426.jpg">Open_Cluster.JPG</basic:xGraphic> + <note>G-Source: http://www.physics.drexel.edu/observatory/dump.shtml</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A group of stars formed together in the spiral + arms of a galaxy.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>open cluster</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>preferredTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>Over 1100 open clusters are known in our Milky + Way Galaxy, and this is probably only a small percentage of the + total population which is probably some factor higher; estimates of + as many as about 100,000 Milky Way open clusters have been given. </basic:context> + <basic:source>http://seds.org/MESSIER/open.html</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>galactic cluster</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>supersededTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>In contrast, the galactic cluster represented by + M29 is a grouping of stars—a “knot” of stars in the stellar + backdrop.</basic:context> + <basic:source>http://www.eastbayastro.org/2000/0900/r0900-8.htm</basic:source> + </descripGrp> + <note>Another name for an open star cluster. They are often termed Galactic + Clusters because they are found mainly in the plane of our galaxy. If + you were to view our galaxy from afar, you would find that all the + open/galactic clusters lie within the spiral arms of the galaxy.</note> + <note>N-Source: + http://www.delscope.demon.co.uk/astronomy/glossary.htm#G</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Una acumulación de una docena hasta varios miles + de jóvenes estrellas en el plano de las galaxias.</basic:definition> + <basic:source>http://www.espacioprofundo.com.ar/diccionario/Glosario_de_Astronomia/vertermino/Cumulo_abierto.html</basic:source> + </descripGrp> + <termSec> + <term>cúmulo abierto</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>M7 es uno de los cúmulos abiertos estelares más + prominentes del cielo. El cúmulo, dominado por brillantes estrellas + azules, puede ser visto a ojo desnudo en un cielo oscuro en la cola + de la constelación del Escorpión (Scorpius).Contiene unas 100 + estrellas en total, tiene una edad aproximada de 200 millones de + años, mide 25 años luz de ancho, y se encuentra a unos 1000 años luz + de distancia.</basic:context> + <basic:source>http://observatorio.info/2009/11/m7-cumulo-abierto-en-scorpius-2/</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c2"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>Stellar Birth</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Accretion_disk#/media/File:Star_with_accretion_disk.jpg">Accretion_Disk.jpg</basic:xGraphic> + <note>G-Source: + http://www.cfht.hawaii.edu/Instruments/Spectroscopy/Espadons/www.ast.obs-mip.fr/users/donati/press/fuori_eng.html</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A structure that forms around a compact object + (e.g. a white dwarf, neutron star, or black hole) when matter flows + towards it.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>circumstellar accretion disk</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>preferredTerm-admn-sts</min:administrativeStatus> + <basic:termType>fullForm</basic:termType> + <descripGrp> + <basic:context>In contrast with the violence of merging, the + gradual growth of massive stars by accretion is likely to produce + less infrared variability, relatively thin circumstellar accretion + disks that maintain their orientation, and collimated bipolar + outflows that are scaled-up versions of those produced by low-mass + young stellar objects.</basic:context> + <basic:source>Bally2005</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>accretion disc</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>Accretion Disc Evolution in Single and Binary T + Tauri Stars</basic:context> + <basic:source>http://cdsweb.cern.ch/record/369655</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>circumstellar disk</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>Our results suggest a scenario of a central star + accreting material from a circumstellar disc at the centre of a cool + extended rotating torus, while driving a fast bipolar wind. </basic:context> + <basic:source>http://adsabs.harvard.edu/abs/2010MNRAS.402.1504D</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Una estructura en forma de disco alrededor de un + objeto central masivo que alimenta el cuerpo central siendo atraido por + éste y contribuye a su aumento de masa.</basic:definition> + <basic:source>http://es.wikipedia.org/wiki/Disco_de_acreci%C3%B3n</basic:source> + </descripGrp> + <termSec> + <term>disco de acreción</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>preferredTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>Lo que alimenta esta actividad es el gas + extraído de la estrella normal, que, cayendo en espiral hacia el + agujero negro, se acumula en un denso disco de acreción.</basic:context> + <basic:source>http://www.amazings.com/ciencia/noticias/010210e.html</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>disco de acrecimiento</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>Imágenes de estrellas jóvenes con discos de + acrecimeinto y chorros colimados de material, tomadas con el + telescopio espacial Hubble.</basic:context> + <basic:source>http://www.laeff.inta.es/index.php?op=modload&name=phpWiki&file=index&pagename=Research-Brown%20Dwarfs-BD_esp-DiscosAcrecimiento</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c3"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>Stellar Death</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Black_hole#/media/File:BH_LMC.png">Black_Hole.jpg</basic:xGraphic> + <note>G-Source: http://wallpaper-s.org/12__Supermassive_Black_Hole.htm</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A region of space where the gravitational force + is so strong that not even light can escape from it.</basic:definition> + <basic:source>Cambridge2007</basic:source> + </descripGrp> + <termSec> + <term>black hole</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>As matter spirals toward and into the black + hole, some of its gravitational potential energy may be efficiently + converted into relativistic jets launched by the magnetic field + along the spin axis.</basic:context> + <basic:source>Bally2005</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Un punto super-denso en el espacio formado por el + colapso de una estrella donde nada puede escapar de su influencia + gravitacional. </basic:definition> + <basic:source>www.atlasoftheuniverse.com/espanol/glossary.html</basic:source> + </descripGrp> + <termSec> + <term>agujero negro</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>En teoría un agujero negro se origina hacia el + final de la vida de una estrella, cuando ésta se contrae mas allá de + un límite determinado - conocido como radio de Schwarzschild - y se + hace más pequeña y mas densa que una estrella de neutrones, tanto + que ni la luz puede escapar de su campo gravitatorio.</basic:context> + <basic:source>http://html.rincondelvago.com/agujeros-negros_5.html</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c4"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Gamma-ray_burst#/media/File:GRB080319B_illustration_NASA.jpg">Gamma_Ray_Burst.jpg</basic:xGraphic> + <note>G-Source: + http://nakedmaninthetree.wordpress.com/2009/02/22/galaxies-and-the-future/</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A temporary intese burst of gamma rays and X-rays + from a cosmic source.</basic:definition> + <basic:source>Cambridge2007</basic:source> + </descripGrp> + <termSec> + <term>gamma-ray burst</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <basic:termType>fullForm</basic:termType> + <descripGrp> + <basic:context>The extremely rare merger of two stars close to + the upper-mass end of the initial mass function may be a possible + pathway to hypernova-generated gamma-ray bursts.</basic:context> + <basic:source>Bally2005</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>GRB</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <basic:termType>acronym</basic:termType> + <descripGrp> + <basic:context>The off-axis collisions and merging of stars + near the top of the stellar mass spectrum may result in the + production of GRBs.</basic:context> + <basic:source>Bally2005</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Destellos de rayos gamma que pueden durar desde + unos nanosegundos hasta cerca de una hora.</basic:definition> + <basic:source>http://es.wikipedia.org/wiki/Brote_de_rayos_gamma</basic:source> + </descripGrp> + <termSec> + <term>explosión de rayos gamma</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Una poderosa explosión de rayos gamma, detectada + el 19 de marzo por el satélite Swift, de la NASA, batió el récord + como el objeto más distante que se pudo observar a simple + vista.</basic:context> + <basic:source>http://ciencia.nasa.gov/headlines/y2008/21mar_nakedeye.htm</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>brote de rayos gamma</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>John Ellis (entrevistado por Punset en su + despacho en el CERN en un programa de Redes) y sus colaboradores + mostraron cómo utilizar las propiedades de los grandes brotes de + rayos gamma (gamma-ray bursters o GRBs) para responder a esta + cuestión.</basic:context> + <basic:source>http://francisthemulenews.wordpress.com/2009/02/21/el-mayor-brote-de-rayos-gamma-grb-080916c-acerca-la-gravedad-cuantica-al-mundo-de-planck/</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c5"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Globular_cluster#/media/File:A_Swarm_of_Ancient_Stars_-_GPN-2000-000930.jpg">Globular_Cluster.jpg</basic:xGraphic> + <note>G-Source: http://www.astrographics.com/GalleryPrintsIndex/GP0046.html</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A roughly spherical group of old stars in the + halo of the galaxy.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>globular cluster</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Although the standard accretion scenario may + well explain the formation of most massive stars, the existence of + blue stragglers in globular clusters indicates that mergers do occur + in nature.</basic:context> + <basic:source>Birth of High-Mass Stars</basic:source> + </descripGrp> + <note>Related Term: star cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Un tipo de cúmulo estelar que consiste en una + agrupación de miles de estrellas viejas, gravitacionalmente ligadas, con + distribución aproximadamente esférica, y que orbita en torno a una + galaxia de manera similar a un satélite.</basic:definition> + <basic:source>http://es.wikipedia.org/wiki/C%C3%BAmulo_globular</basic:source> + </descripGrp> + <termSec> + <term>cúmulo globular</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context> De los 200 cúmulos globulares que sobreviven + hoy, M3 es uno de los más grande y luminoso, fácilmente observable + con binoculares en el hemisferio Norte del cielo.</basic:context> + <basic:source>http://www.tayabeixo.org/portadas/m3.htm</basic:source> + </descripGrp> + <note>Related Term: cúmulo estelar</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c6"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Main_sequence#/media/File:HRDiagram.png">Main_Sequence.jpg</basic:xGraphic> + <note>G-Source: http://www.skyofplenty.com/?page_id=374</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Of or dealing with a major group of stars forming + a band stretching from upper left to lower right on a + Hertzsprung-Russell diagram when being plotted by luminosity and surface + temperature.</basic:definition> + <basic:source>http://en.wiktionary.org/wiki/main-sequence</basic:source> + </descripGrp> + <termSec> + <term>main-sequence</term> + + + <min:partOfSpeech>adjective</min:partOfSpeech> + <descripGrp> + <basic:context>However, immediately after its formation, the + merger product is likely to have a photospheric radius considerably + larger than that of a main-sequence star with the same + mass.</basic:context> + <basic:source>Bally2005</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Pertenece a las estrellas en la región del + diagrama de Hertzsprung-Russell en la que se encuentran la mayor parte + de las estrellas que transforman hidrógeno en helio.</basic:definition> + <basic:source>http://es.wikipedia.org/wiki/Secuencia_principal</basic:source> + </descripGrp> + <termSec> + <term>de secuencia principal</term> + + + <min:partOfSpeech>adjective</min:partOfSpeech> + <descripGrp> + <basic:context>Por ejemplo, nuestro sol es una estrella de + secuencia principal regular de tamaño pequeño. </basic:context> + <basic:source>http://celestia.albacete.org/celestia/celestia/stars/secu5.htm</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c7"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>Stellar Birth</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Protostar#/media/File:A_diamond_in_the_dust.jpg">Protostar.JPG</basic:xGraphic> + <note>G-Source: http://www.konkoly.hu/KISAG/Science/star/star_intro.html</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A star in the earliest observable stage of + formation.</basic:definition> + <basic:source>Cambridge2007</basic:source> + </descripGrp> + <termSec> + <term>protostar</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Alternatively, it has been suggested that + massive stars form from the merging of lower mass protostars in + high-density protostar clusters (Bonnell et al.1998; Stahler et al. + 2000; Bonnell 2002; Zinnecker & Bate 2002).</basic:context> + <basic:source>Bally2005</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Una región muy densa o descorazonada de nubes + moleculares donde existen estrellas en proceso de formación.</basic:definition> + <basic:source>www.astrocosmo.cl/glosario/glosar-p.htm</basic:source> + </descripGrp> + <termSec> + <term>protoestrella</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>En estos primeros estadios, la protoestrella es + un objeto muy activo, y produce un viento bipolar formado por dos + chorros opuestos de material de alta velocidad. </basic:context> + <basic:source>http://www.fomento.es/MFOM/LANG_CASTELLANO/DIRECCIONES_GENERALES/INSTITUTO_GEOGRAFICO/Astronomia/InvestermSecacion/astronomia/protoestrellas.htm</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c8"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Star_cluster#/media/File:M92_arp_750pix.jpg">Star_Cluster.jpg</basic:xGraphic> + <note>G-Source: http://apod.nasa.gov/apod/ap060109.html</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A collection of stars formed together from the + same gas cloud and bound together by mutual gravitational + attraction.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>star cluster</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Most star clusters are too far away and the + white dwarfs are too faint to be seen by ground-based telescopes, + but Hubble's powerful vision sees many of them.</basic:context> + <basic:source>http://hubblesite.org/newscenter/archive/releases/star%20cluster/2008/25/full/</basic:source> + </descripGrp> + <note>Related Term: globular cluster</note> + <note>Related Term: open cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Un grupo de estrellas atraídas entre sí por su + gravedad mutua.</basic:definition> + <basic:source>http://iopscience.iop.org/1538-3881/129/5/2281/pdf/1538-3881_129_5_2281.pdf</basic:source> + </descripGrp> + <termSec> + <term>cúmulo estelar</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>preferredTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>“Es como encontrar un pez fuera del agua”, dice + Ed Churchwell, profesor de astronomía de la Universidad de + Wisconsin-Madison, quien con un equipo de científicos de UW-Madison, + de la Universidad de Wyoming, de la Universidad de Boston, del + Instituto de Ciencia Espacial de Boulder, Colorado, y del Centro de + Ciencia Spitzer descubrieron este inusual cúmulo estelar con la + ayuda del Telescopio Espacial Spitzer de la NASA. </basic:context> + <basic:source>http://www.astroseti.org/vernew.php?codigo=1117</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>cúmulo de estrellas</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>Los cúmulos de estrellas se clasifican en dos + grupos: cúmulos abiertos, que no poseen forma definida, y cúmulos + globulares, que son esféricos o casi esféricos.</basic:context> + <basic:source>http://www.astromia.com/universo/cumulos.htm</basic:source> + </descripGrp> + <note>Related Term: cúmulo globular</note> + <note>Related Term: cúmulo abierto</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c9"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Milky_Way#/media/File:ESO-VLT-Laser-phot-33a-07.jpg">Milky_Way.jpg</basic:xGraphic> + <note>G-Source: http://www.cfa.harvard.edu/~afrebel/milky-way-2.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A band of faint light across the sky, visible to + the naked eye on a moonless night, consisting of stars and glowing gas + in the disk of our own Galaxy.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>Galaxy</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <basic:termType>shortForm</basic:termType> + <descripGrp> + <basic:context>If merging is an important pathway to the + formation of massive stars, then it is expected that some + highluminosity IRAS sources in our Galaxy have brightened or faded + since the IRAS observations were made.</basic:context> + <basic:source>Bally2005</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>Milky Way Galaxy</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <basic:termType>fullForm</basic:termType> + </termSec> + <termSec> + <term>Milky Way</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <basic:termType>shortForm</basic:termType> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Una galaxia espiral en la que se encuentra el + Sistema Solar y, por ende, la Tierra.</basic:definition> + <basic:source>http://es.wikipedia.org/wiki/Vía_Láctea</basic:source> + </descripGrp> + <termSec> + <term>Galaxia</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <basic:termType>shortForm</basic:termType> + <descripGrp> + <basic:context>La Vía Láctea, también llamada la Galaxia, es un + agrupamiento de estrellas con forma de disco, que incluye al Sol y a + su sistema solar.</basic:context> + <basic:source>www.todoelsistemasolar.com.ar/vlactea.htm</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>Vía Láctea</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <basic:termType>shortForm</basic:termType> + <descripGrp> + <basic:context>La Via Láctea és una galaxia grande, espiral y + puede tener unos 100.000 millones de estrellas, entre ellas, el Sol. </basic:context> + <basic:source>http://www.astromia.com/universo/vialactea.htm</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>galaxia Vía Láctea</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <basic:termType>fullForm</basic:termType> + <descripGrp> + <basic:context>La galaxia Vía Láctea es una galaxia espiral que + es nuestro hogar, al igual que el de otras 100 mil millones + estrellas. </basic:context> + <basic:source>http://www.windows.ucar.edu/tour/link=/the_universe/Milkyway.sp.html</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c10"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Star#/media/File:The_Sun_by_the_Atmospheric_Imaging_Assembly_of_NASA%27s_Solar_Dynamics_Observatory_-_20100819.jpg">Star.jpg</basic:xGraphic> + <note>G-Source: + http://lh4.ggpht.com/_EuutPdvjcY0/SQ2jGBKWO7I/AAAAAAAAALM/gjDMVimDQc8/005Est.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A large, luminous ball of gas generating energy + internally by nuclear fusion.</basic:definition> + <basic:source>Cambridge2007</basic:source> + </descripGrp> + <termSec> + <term>star</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>While the behavior of stars forming by accretion + is reasonably well understood,the consequences of merging have not + been fully investermSecated.</basic:context> + <basic:source>Bally2005</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Una enorme y densa bola de gas que genera fusión + nuclear, liberando así una gran cantidad de energía</basic:definition> + <basic:source>spaceplace.nasa.gov/sp/kids/spitzer/signs/sign_glossary.shtml</basic:source> + </descripGrp> + <termSec> + <term>estrella</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Las estrellas son enormes aglomeraciones de gas, + principalmente Hidrogeno, cuya temperatura es tan alta debido a la + fusión de este elemento, que irradian luz a lo largo de todo el + espectro electromagnético. Poseen diferentes temperaturas que varían + desde los 2000 grados Celsius hasta los 50000.</basic:context> + <basic:source>http://www.astrosurf.com/astronosur/estrellas.htm</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c11"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Ultraviolet#/media/File:UV_LED_Fluoresence.jpg">UV_Radiation.jpg</basic:xGraphic> + <note>G-Source: http://drdima.files.wordpress.com/2009/05/sun-rays.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>The region of the electromagnetic spectrum + spanning the wavelength range from the Lymann limit at 91.2 nm to 350 + nm.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>UV radiation</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <basic:termType>shortForm</basic:termType> + <descripGrp> + <basic:context>UV radiation from stars and shocks likely + provide the minimum level of ionization required to couple these + fields strongly to the entangled medium.</basic:context> + <basic:source>Bally2005</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>ultraviolet radiation</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <basic:termType>fullForm</basic:termType> + <descripGrp> + <basic:context>Ultraviolet (UV) radiation is part of the + electromagnetic spectrum emitted by the sun. </basic:context> + <basic:source>http://www.who.int/uv/en/</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>La radiación electromagnética cuya longitud de + onda está comprendida aproximadamente entre los 400 nm y los 15 + nm.</basic:definition> + <basic:source>http://es.wikipedia.org/wiki/Radiaci%C3%B3n_UV</basic:source> + </descripGrp> + <termSec> + <term>radiación UV</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <basic:termType>shortForm</basic:termType> + <descripGrp> + <basic:context>Los usuarios de camas solares se someten a dosis + considerables de radiaciones UV artificiales para conseguir un + bronceado complementario al obtenido al tomar el sol.</basic:context> + <basic:source>http://copublications.greenfacts.org/es/camas-solares/</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>radiación ultravioleta</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <basic:termType>fullForm</basic:termType> + <descripGrp> + <basic:context>La radiación ultravioleta se encuentra entre la + luz visible y los rayos X del espectro electromagnético.</basic:context> + <basic:source>http://www.windows.ucar.edu/tour/link=/physical_science/magnetism/em_ultraviolet.sp.html</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c12"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Magnetic_field#/media/File:VFPt_magnets_BHM.svg">Magnetic_Field.jpg</basic:xGraphic> + <note>G-Source: http://www.greatdreams.com/magnet1.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A region subject to the influence of magnetism + that is manifested by the mechanical forces that it exerts upon + electricity moving across it and upon the poles of magnets placed in + it.</basic:definition> + <basic:source>Merriam-Webster2002</basic:source> + </descripGrp> + <termSec> + <term>magnetic field</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Detailed consideration of the merger process + will require numerical modeling in which the hydrodynamics, effects + of gravity,magnetic fields, and radiation are considered + carefully.</basic:context> + <basic:source>Bally2005</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Un campo de fuerza creado como consecuencia del + movimiento de cargas eléctricas, del flujo de la electricidad.</basic:definition> + <basic:source>http://www.greenfacts.org/es/glosario/abc/campo-magnetico.htm</basic:source> + </descripGrp> + <termSec> + <term>campo magnético</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>El campo magnético es producido por la corriente + eléctrica que circula por un conductor.</basic:context> + <basic:source>http://teleformacion.edu.aytolacoruna.es/FISICA/document/teoria/A_Franco/elecmagnet/magnetico/cMagnetico.html</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c13"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Blue_straggler#/media/File:Ngc6397_hst_blue_straggler.jpg">Blue_Straggler.jpg</basic:xGraphic> + <note>G-Source: http://images.spaceref.com/news/2009/ooBlue_Straggler09.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A blue main-sequence star, usually found in a + globular or open cluster that appears to be slower in its evolution than + other stars of similar mass and luminosity in the same + cluster.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>blue straggler</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Numerical models of stellar collisions leading + to the formation of blue stragglers in globular clusters (Lombardi + et al. 2002, 2003; Fregeau et al. 2004) indicate that merger + products have radii up to 30 times larger than that of an equivalent + main-sequence star.</basic:context> + <basic:source>Bally2005</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Estrellas que aparentan una edad menor que la del + sistema estelar al que pertenecen, si se supone que se formaron junto + con él.</basic:definition> + <basic:source>http://es.wikipedia.org/wiki/Estrella_rezagada_azul</basic:source> + </descripGrp> + <termSec> + <term>estrella rezagada azul</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>preferredTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>Las últimas observaciones de las “rezagadas + azules”, estrellas atípicas que aparentan ser más jóvenes que el + sistema estelar al que pertenecen, han proporcionado dos modelos + diferentes sobre su origen.</basic:context> + <basic:source>http://mundoastronomia.portalmundos.com/nuevas-pistas-sobre-el-origen-de-las-estrellas-rezagadas-azules/</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c14"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>The sudden collapse of a massive star when the + internal pressure pushing outwards falls so that it cannot balance the + weight of material pressing inward.</basic:definition> + <basic:source>Cambridge2007</basic:source> + </descripGrp> + <termSec> + <term>gravitational collapse</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Stars form from the gravitational collapse of + turbulent molecular cloud cores (Elmegreen & Scalo 2004; Mac Low + & Klessen 2004).</basic:context> + <basic:source>Bally2005</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>El estado final de la evolución de una estrella + de gran masa en el que la materia se comprime bajo la acción de su + propia atracción gravitatoria, con desprendimiento de grandes cantidades + de energía.</basic:definition> + <basic:source>http://www.conocimientosweb.net/portal/term6172.html</basic:source> + </descripGrp> + <termSec> + <term>colapso gravitacional</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Esto sucede si la masa de un pedazo de la nube + excede cierto valor crítico, de modo tal que la fuerza de gravedad + vence definitivamente y el pedazo empieza a contraerse, aumentando + su densidad. Este proceso se llama colapso gravitacional. </basic:context> + <basic:source>http://bibliotecadigital.ilce.edu.mx/sites/ciencia/volumen1/ciencia2/06/html/sec_15.html</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c15"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Binary_star#/media/File:Algol_AB_movie_imaged_with_the_CHARA_interferometer_-_labeled.gif">Binary_Star.jpg</basic:xGraphic> + <note>G-Source: + http://lh6.ggpht.com/_6hgSmco4R9M/SaqplXGqJfI/AAAAAAAAA1k/B3a43_O9VI8/56_Binary_Stars_thumb3.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A pair of stars in orbit around each other, held + together by the graviational attraction between them.</basic:definition> + <basic:source>Cambridge2007</basic:source> + </descripGrp> + <termSec> + <term>binary star</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>These authors considered collision partners + having similar masses and concluded that such interactions can at + most account for a small fraction of the observed binary star + population in young clusters.</basic:context> + <basic:source>Bally2005</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Un sistema estelar compuesto de dos estrellas que + orbitan mutuamente alrededor de un centro de masas común.</basic:definition> + <basic:source>http://es.wikipedia.org/wiki/Estrella_binaria</basic:source> + </descripGrp> + <termSec> + <term>estrella binaria</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>La explosión de una estrella binaria dentro de + una nebulosa planetaria ha sido capturado por un equipo dirigido por + investermSecadores del University College of London UCL - es un + acontecimiento que no ha sido presenciado hace más de 100 + años.</basic:context> + <basic:source>http://www.astroelche.es/blog/index.php?blog=2&title=astronomos-capturam-la-explosion-de-una-&more=1&c=1&tb=1&pb=1</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>estrella doble</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>preferredTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>Una estrella doble es una pareja de estrellas + que se mantienen unidas por la fuerza de la gravitación y giran en + torno a su centro común.</basic:context> + <basic:source>http://www.astromia.com/universo/dobles.htm</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c16"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>Stellar Birth</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Initial_mass_function#/media/File:LH_95.jpg">Initial_Mass_Function.JPG</basic:xGraphic> + <note>G-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <note>This figure compares the IMFs by ploting mass fraction per dex versus mass, + i.e., normalized so that the integral under each curve is unity. They are + assumed to be valid from 0.1 to 120 solar masses.</note> + <note>N-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A mathematical description of the relative + frequncy with which stars of various masses are formed.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>initial mass function</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>The extremely rare merger of two stars close to + the upper-mass end of the initial mass function may be a possible + pathway to hypernova-generated gamma-ray bursts.</basic:context> + <basic:source>Bally2005</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-17</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>La expresión numérica que determina el número de + estrellas con masa en un rango determinado.</basic:definition> + <basic:source>Basado en http://laeff.cab.inta-csic.es/modules.php?op=modload&name=phpWiki&file=index&pagename=Research-Estrellas-IMF</basic:source> + </descripGrp> + <termSec> + <term>función inicial de masa</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Estado evolutivo y función inicial de masa de + cúmulos jóvenes en la gran nube de Magallanes (estudio en el + ultravioleta).</basic:context> + <basic:source>http://dialnet.unirioja.es/servlet/tesis?codigo=11651</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c17"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <termSec> + <term>Bally2005</term> + + + <note>Author[s]: Bally, John and Hans Zinnecker</note> + <note>Journal Title: The Astronomical Journal</note> + <note>Article Title: The Birth of High-Mass Stars: Accertion and/or + Mergers?</note> + <note>Volume: 129</note> + <note>Publication Place: U.S.A.</note> + <note>Publisher: The American Astronomical Society</note> + <note>Publication Year: May 2005</note> + <note>Page(s): 2281-2293</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c18"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <termSec> + <term>Cambridge2007</term> + + + <note>Author[s]: Mitton, Jaqueline</note> + <note>Book Title: Cambridge Illustrated Dictionary of Astronomy</note> + <note>Publication Place: New York</note> + <note>Publisher: Cambridge University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c19"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <termSec> + <term>Merriam-Webster2002</term> + + + <note>Book Title: Webster's Third New International Dictionary</note> + <note>Editor[s]: Gove, Philip Babcock</note> + <note>Volume: Third Edition</note> + <note>Publication Place: Springfield, Massachusetts</note> + <note>Publisher: Merriam-Webster INC.</note> + <note>Publication Year: 2002</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c20"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <termSec> + <term>Oxford2007</term> + + + <note>Book Title: Oxford Dictionary of Astronomy</note> + <note>Editor[s]: Ridpath, Ian</note> + <note>Volume: Second Edition</note> + <note>Publication Place: New York</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c21"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>Stellar Death</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Supernova#/media/File:SN1994D.jpg">Supernova.jpg</basic:xGraphic> + <note>G-Source: + http://jcconwell.wordpress.com/2009/07/24/top-10-ways-the-universe-could-kill-us/supernova/</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A catastrophic stellar explosion in which so much + energy is released that the supernova alone can outshine an entire + galaxy of billions of stars.</basic:definition> + <basic:source>Cambridge2007</basic:source> + </descripGrp> + <termSec> + <term>supernova</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>The supermassive object may be eventually + disrupted by an unusually violent supernova explosion (a hypernova) + soon after formation.</basic:context> + <basic:source>Bally2005</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-20</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Una estrella que estalla y lanza a todo su + alrededor la mayor parte de su masa a altísimas velocidades.</basic:definition> + <basic:source>http://www.astromia.com/glosario/supernova.htm</basic:source> + </descripGrp> + <termSec> + <term>supernova</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Un equipo de científicos británicos propone esta + semana en la revista Nature que la tenue supernova SN2008ha, + descubierta por una adolescente estadounidense en noviembre de 2008, + podría ser la explosión de una estrella masiva, en lugar de proceder + de una enana blanca como se planteaba hasta ahora.</basic:context> + <basic:source>http://www.plataformasinc.es/index.php/esl/Noticias/Una-supernova-observada-por-astronomos-aficionados-abre-el-debate-entre-los-profesionales</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c22"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <termSec> + <term>Moore2003</term> + + + <note>Author[s]: Moore, Patrick</note> + <note>Book Title: Philip's Atlas of the Universe</note> + <note>Publication Place: Heron Quays, London</note> + <note>Publisher: Philip's</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c23"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Red_giant#/media/File:Mira_1997.jpg">Red_Giant.jpg</basic:xGraphic> + <note>G-Source: + http://www.lcsd.gov.hk/CE/Museum/Space/EducationResource/Universe/framed_e/lecture/ch15/imgs/red_size.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A cool, large and highly luminous star that has + left the main sequence and is powered by heavier elements than + hydrogen.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>red giant</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>The core temperature becomes so high that helium + start to 'burn', producing carbon; around this active core there is + a shell where hydrogen is still producing energy. The star becomes + unstable, and the outer layers swell out, cooling as they do so. The + star becomes a red giant.</basic:context> + <basic:source>Moore2003</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Una estrella de masa baja o intermedia (menos de + 8-9 masas solares) que, tras haber consumido el hidrógeno en su núcleo + durante la etapa de secuencia principal, convirtiéndolo en helio por + fusión nuclear, comienza a quemar hidrógeno en una cáscara alrededor del + núcleo de helio inerte.</basic:definition> + <basic:source>http://es.wikipedia.org/wiki/Gigante_roja</basic:source> + </descripGrp> + <termSec> + <term>gigante roja</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>La gigante roja S Orionis (S Ori) es una + estrella variable del tipo Mira. Su masa es similar a la del Sol, + con la diferencia de que está mucho más cerca de convertirse en una + enana blanca, el mismo final que le espera a nuestro Sol dentro de 5 + mil millones de años.</basic:context> + <basic:source>http://www.solociencia.com/astronomia/07071709.htm</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c24"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Red_dwarf#/media/File:New_shot_of_Proxima_Centauri,_our_nearest_neighbour.jpg">Red_Dwarf.jpg</basic:xGraphic> + <note>G-Source: http://www.wolflodge.org/bluestar/h_red_dwarf_02.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A cool, faint, low-mass star lying at the lower + end of the main sequence of spectral type K or M.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>red dwarf</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>The dim red dward Proxima, more than a degree + away from Alpha, is slightly closer to us.</basic:context> + <basic:source>Moore2003</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Una estrella pequeña y relativamente fría de la + secuencia principal, ya sea de tipo espectral K tardío o M.</basic:definition> + <basic:source>http://es.wikipedia.org/wiki/Enana_roja</basic:source> + </descripGrp> + <termSec> + <term>enana roja</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>El planeta que se ha descubierto girando + alrededor de esta enana roja tiene una masa equivalente a la de + Neptuno, es decir, es sólo 17 veces mayor que la Tierra y mucho + menor que Saturno.</basic:context> + <basic:source>http://axxon.com.ar/not/157/c-1570034.htm</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c25"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Stellar_classification#/media/File:Zeta_Puppis.png">Spectral_Type.jpg</basic:xGraphic> + <note>G-Source: + http://www.astro.columbia.edu/~archung/labs/spring2002/images/spectral_type2.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A means of classifying stars according to the + details of their spectrum, depending largely on their surface + temperature.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>spectral type</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>In this version of a typical HR diagram, the + stars are plotted according to their spectral types and suface + temperatures (horzontal axis, x) and their luminositites in therms + of the Sun (vertical axis, y).</basic:context> + <basic:source>Moore2003, 171</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>El espectro de una estrella clasificado por una + letra (O, B, A, F, G, K, M, R, N, S) seguida de un digito que describe + el color de la estrella y su temperatura.</basic:definition> + <basic:source>Basado en http://www.espacioprofundo.com.ar/diccionario/Glosario_de_Astronomia/vertermino/Tipo_espectral.html</basic:source> + </descripGrp> + <termSec> + <term>tipo espectral</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>En el gráfico superior se muestra la intensidad + de las líneas espectrales según la temperatura de la estrella (tipo + espectral)</basic:context> + <basic:source>http://www.astrosurf.com/astronosur/estrellas.htm</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c26"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/White_dwarf#/media/File:Sirius_A_and_B_Hubble_photo.editted.PNG">White_Dwarf.jpg</basic:xGraphic> + <note>G-Source: http://www.stsci.edu/~inr/thisweek1/thisweek/WhiteDwarf.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A small dense star that is has run out of fuel + for nuclear fusion, collapsing under its own gravity and blowing off its + outer layers to form a planetary nebula in the process.</basic:definition> + <basic:source>Based on Oxford2007 and Cambridge2007</basic:source> + </descripGrp> + <note>This is the end-result of all but the most massive of stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>white dwarf</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>To the upper right lie giants and supergiants of + tremendous luminosity, while to the lower left there are the white + dwarfs, which are in a differnt category and were not known when HR + Diagrams were introduced.</basic:context> + <basic:source>Moore2003, 170</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Un remanente estelar que se genera cuando una + estrella de masa menor a 9-10 masas solares ha agotado su combustible + nuclear.</basic:definition> + <basic:source>http://es.wikipedia.org/wiki/Enana_blanca</basic:source> + </descripGrp> + <termSec> + <term>enana blanca</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Cuando el material fusionable se agota la + estrella pierde la presión interna producida por la fusión nuclear y + puede colapsar inmediatamente terminando en una enana + blanca.</basic:context> + <basic:source>http://astroverada.com/_/Main/T_evolucion.html</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c27"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Planetary_nebula#/media/File:NGC6543.jpg">Planetary_Nebula.jpg</basic:xGraphic> + <note>G-Source: + http://www.phys.ncku.edu.tw/~astrolab/mirrors/apod_e/image/0901/ngc2818_hheritage_800.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A bright cloud of glowing gas and dust + surrounding a highly evolved star.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <note>As mass is gradually lost, the core of the star becomes more exposed, + ultimately becoming a white dwarf. Also, planetary nebulae have nothing to + do with planets, and are not true nebulae.</note> + <note>N-Source: Based on Oxford2007 and Moore2003, 186</note> + <termSec> + <term>planetary nebula</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>The star's outer layers are thrown off, and for + a cosmically brief period - no more than about 100,000 years - we + have the phenomenon of what is termed a planetary nebula.</basic:context> + <basic:source>Moore2003, 173</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Una nebulosa de emisión consistente en una + envoltura brillante en expansión de plasma y gas ionizado, expulsada + durante la fase de rama asintótica gigante que atraviesan las estrellas + gigantes rojas en los últimos momentos de sus vidas.</basic:definition> + <basic:source>http://es.wikipedia.org/wiki/Nebulosa_planetaria</basic:source> + </descripGrp> + <termSec> + <term>nebulosa planetaria</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Las nebulosas planetarias resultan objetos muy + espectaculares si se observan con un telescopio de media o gran + potencia.</basic:context> + <basic:source>http://www.astromia.com/glosario/nebulosaplanetaria.htm</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c28"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>Stellar Birth</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Emission_nebula#/media/File:Ring_Nebula.jpg">Emission_Nebula.jpg</basic:xGraphic> + <note>G-Source: http://apod.nasa.gov/apod/image/0612/NGC2174_lrg.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A luminous cloud of gas and sust in space which + shines with its own light, which can be generated in several + ways.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <note>Ultraviolet radiation, gas cloud collisions, and synchrotron radiation can + all cause the emission nebula to shine.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>emission nebula</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>preferredTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>In this and other similar emission nebulae, + energetic ultraviolet light from a hot young star strips electrons + from the surrounding hydrogen atoms.</basic:context> + <basic:source>http://apod.nasa.gov/apod/emission_nebulae.html</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Una nube de gas interestelar que brilla por la + excitación del gas, causado por radiación ultravioleta emitida por + estrellas inmersas en la nube o por calentamiento debido a otro + mecanismos. </basic:definition> + <basic:source>http://www.diclib.com/Nebulosa%20de%20emisi%C3%B3n/show/en/es_astronomia/726</basic:source> + </descripGrp> + <termSec> + <term>nebulosa de emisión</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Las nebulosas de emisión estan normalmente en + los lugares de formación de estrellas.</basic:context> + <basic:source>http://www.astrored.net/nebulosaweb/types.html</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c29"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Nebula#/media/File:Eagle_nebula_pillars.jpg">Nebula.jpg</basic:xGraphic> + <note>G-Source: + http://my-blackberry.net/wallpapers/49/m/NASA_-_The_Horsehead_Nebula%2C_B33%2C_Orion_Nebula.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A cloud of interstellar gas and dust.</basic:definition> + <basic:source>Cambridge2007</basic:source> + </descripGrp> + <note>The term was originally applied to any object with a fuzzy telescopic + appearance, but with the advent of larger instruments many 'nebulae' were + found to consist of faint stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>nebula</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <note>Grammatical Number: singular</note> + <descripGrp> + <basic:context>According to current theory, a star begins by + condensing out of the tenuous material making up a nebula.</basic:context> + <basic:source>Moore2003, 172</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>nebulae</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <note>Grammatical Number: plural</note> + <descripGrp> + <basic:context>Other nebulae are within the range of small + telescopes.</basic:context> + <basic:source>Moore2003, 187</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-24</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Regiones del medio interestelar constituidas por + gases (principalmente hidrógeno y helio) y polvo.</basic:definition> + <basic:source>http://es.wikipedia.org/wiki/Nebulosa</basic:source> + </descripGrp> + <termSec> + <term>nebulosa</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>A unos 1.500 años-luz de distancia, dentro de + nuestro brazo espiral en la Vía Láctea, la Nebulosa de Orión está en + el centro de la región de la Espada de la constelación de Orión el + Cazador, que domina el cielo nocturno a inicios del invierno, en las + latitudes Norte.</basic:context> + <basic:source>http://www.oarval.org/OrionNebsp.htm</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c30"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-28</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>Stellar Birth</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Dark_nebula#/media/File:All_Quiet_in_the_Nursery%3F.jpg">Dark_Nebula.jpg</basic:xGraphic> + <note>G-Source: http://www.mallorcaweb.net/masm/obstel/caballo.GIF</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-28</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-28</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-28</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-28</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A type of interstellar cloud that is so dense + that it obscures the light from the background emission or reflection + nebula or that it blocks out background stars.</basic:definition> + <basic:source>http://en.wikipedia.org/wiki/Dark_nebula</basic:source> + </descripGrp> + <termSec> + <term>dark nebula</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>preferredTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>There is no difference between a dark nebula and + a bright one, except for the lack of illumination.</basic:context> + <basic:source>Moore2003, 187</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>absorbtion nebula</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>An absorption nebula is a dense cloud of dust + and gas. From the point of view of an observer on Earth, it absorbs + the light from more distant stars, creating a dark, starless + region.</basic:context> + <basic:source>http://www.glyphweb.com/esky/concepts/absorptionnebula.html</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-28</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-28</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-28</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-28</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Nubes de polvo que simplemente tapan la luz de lo + que haya detras.</basic:definition> + <basic:source>http://www.astrored.net/nebulosaweb/types.html</basic:source> + </descripGrp> + <termSec> + <term>nebulosa oscura</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>preferredTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>Aqui hay un mapa que muestra las regiones de + nebulosas oscuras que estan en un radio de 2000 años luz.</basic:context> + <basic:source>http://www.atlasoftheuniverse.com/espanol/darknebs.html</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>nebulosa de absorción</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>El caso más opuesto a las nebulosas de emisión + son las nebulosas de absorción (nebulosas oscuras). Estas ni si + quiera están rodeadas de estrellas lo suficientemente potentes ni + cercanas para hacer llegar la luminosidad suficiente para que la + nebulosa pueda reflejarla.</basic:context> + <basic:source>http://www.blogdeastronomia.es/astronomia/formacion-de-estrellas/las-nebulosas</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c31"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-28</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-28</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>Stellar Birth</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Reflection_nebula#/media/File:Reflection.nebula.arp.750pix.jpg">Reflection_Nebula.jpeg</basic:xGraphic> + <note>G-Source: + http://mm04.nasaimages.org/MediaManager/srvr?mediafile=/Size3/NVA2-8-NA/14107/full_tif.jpg&userid=1&username=admin&resolution=3&servertype=JVA&cid=8&iid=NVA2&vcid=NA&usergroup=HUBBLE&profileid=39</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-28</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-28</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A cloud of interstellar gas and dust that appears + bight because it reflects or scatters starlight.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>reflection nebula</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Just weeks after NASA astronauts repaired the + Hubble Space Telescope in December 1999, the Hubble Heritage Project + snapped this picture of NGC 1999, a reflection nebula in the + constellation Orion. </basic:context> + <basic:source>http://www.nasa.gov/multimedia/imagegallery/image_feature_701.html</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-28</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-28</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Nubes de polvo que simplemente reflejan la luz de + una estrella o estrellas cercanas.</basic:definition> + <basic:source>http://www.astrored.net/nebulosaweb/types.html</basic:source> + </descripGrp> + <termSec> + <term>nebulosa de reflexión</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Como el propio nombre implica, esta nebulosa de + reflexión asociada con la estrella Rigel, se asemeja a una vieja + arpía de un cuento de hadas. </basic:context> + <basic:source>http://www.astrofotos.com.es/2008/11/nebulosa-de-la-cabeza-de-bruja.html</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c32"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Neutron_star#/media/File:PIA18848-PSRB1509-58-ChandraXRay-WiseIR-20141023.jpg">Neutron_Star.jpg</basic:xGraphic> + <note>G-Source: http://nrumiano.free.fr/Images/Neutron_star_E.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <termSec> + <term>neutron star</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>After its Main Sequence period the star becomes + a red supergiant and may explode as a supernova. It may end as a + neutron star or pulsar, although if its mass is even greater it may + poroduce a black hole.</basic:context> + <basic:source>Moore2003, 173</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Un cuerpo pequeño muy denso que se forma en el + envejecimiento de una estrella pesada y que está formada únicamente por + partículas subatómicas denominadas neutrones.</basic:definition> + <basic:source>http://www.astroasa.com.ar/diccionario_astro.htm</basic:source> + </descripGrp> + <termSec> + <term>estrella de neutrones</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>El Gran Telescopio Canarias (GTC), instalado en + el Observatorio del Roque de los Muchachos (La Palma), ha obtenido + imágenes de una profundidad "sin precedentes" de una estrella de + neutrones del tipo magnetar, de las que se conocen seis, según ha + informado el Instituto de Astrofísica de Canarias (IAC).</basic:context> + <basic:source>http://www.rtve.es/noticias/20100301/imagen-unica-estrella-neutrones-cazada-canarias/321412.shtml</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c33"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>Stellar Death</min:subjectField> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>The maximum possible mass of a degenerate star, + above which it will be unable to support itself against the inward pull + of its own gravity. </basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <note>For a star with no hydrogen content the limit is 1.44 solar masses, which + is thus the maximum possible for a white dwarf.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>Chandrasekhar limit</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>However, there is a limit, once the mass of the + white dwarf becomes greater than 1.4 time that of the sun )a value + known as the Chandrasekhar limit, after the Indian astronomer who + first worked it out=, the carbon detonates, and in a matter of a few + seconds the white dwarf blows itself to pieces.</basic:context> + <basic:source>Moore2003</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>El límite de masa más allá del cual la + degeneración de electrones no es capaz de contrarrestar la fuerza de + gravedad en un remanente estelar, produciéndose un colapso que origina + una estrella de neutrones o un agujero negro. </basic:definition> + <basic:source>http://es.wikipedia.org/wiki/L%C3%ADmite_de_Chandrasekhar</basic:source> + </descripGrp> + <termSec> + <term>límite de Chandrasekhar</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Descubrió una masa (aproximadamente 1.5 veces la + masa del Sol) en la que una estrella fría no podría soportar su + gravedad. Esto es lo que se conoce como el límite de + Chandrasekhar.</basic:context> + <basic:source>http://html.rincondelvago.com/agujeros-negros_5.html</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c34"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>Stellar Death</min:subjectField> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>The state of degeneracy attained when the density + of matter is so high that neutrons cannot be packed any more closely + together.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <note>Encountered on in neutron stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>neutron degeneracy</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>When it reaches the threshold of energy + necessary to force the combining of electrons and protons to form + neutrons, the electron degeneracy limit has been passed and the + collapse continues until it is stopped by neutron + degeneracy.</basic:context> + <basic:source>http://hyperphysics.phy-astr.gsu.edu/HBASE/Astro/pulsar.html</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>El estado de degeneración alcanzado cuando la + densidad de materia es tan alta, que los neutrones no pueden juntarse + más.</basic:definition> + <basic:source>Oxford2003</basic:source> + </descripGrp> + <termSec> + <term>degeneración de neutrones</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Es la principal responsable de la resistencia al + colapso gravitacional de las enanas blancas (degeneración de + electrones) y de las estrellas de neutrones (degeneración de + neutrones). </basic:context> + <basic:source>http://www.emiliosilveravazquez.com/glosario.php?letra=d</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c35"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Event_horizon#/media/File:Spacetime_lattice_analogy.svg">Event_Horizon.jpg</basic:xGraphic> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>The radius of the event horizon of a black + hole.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>Schwarzschild radius</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>The critical radius of a non-rotating black hole + is called the Schwarzschild radius, after the German astronomer who + investermSecated the problem mathematically as long ago as 1916: the + boundary around the collapsed star having this radius is termed the + 'event horizon'.</basic:context> + <basic:source>Moore2003</basic:source> + </descripGrp> + <note>Related Term: event horizon</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>El radio del horizonte de sucesos para un agujero + negro.</basic:definition> + <basic:source>http://www.astrocosmo.cl/glosario/glosar-r.htm</basic:source> + </descripGrp> + <termSec> + <term>radio de Schwarzschild</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Me pareció muy interesante este vídeo del + proyecto Sixty Symbols de la Universidad de Nottingham en el que + explican de forma divulgativa qué es el radio de Schwarzschild. + Básicamente es el radio de un agujero negro.</basic:context> + <basic:source>http://www.microsiervos.com/archivo/ciencia/agujeros-negros-y-el-radio-de-schwarzschild.html</basic:source> + </descripGrp> + <note>Related Term: horizonte de sucesos, horizonte de eventos</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c36"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>Stellar Death</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Event_horizon#/media/File:Spacetime_lattice_analogy.svg">Event_Horizon.jpg</basic:xGraphic> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>The surface of a black hole.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>event horizon</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Narayan and Heyl have calculated that if very + heavy objects do not collapse to a point with an event horizon but + instead have a surface, they would eject as many type 1 bursts as + neutron stars.</basic:context> + <basic:source>http://www.newscientist.com/article/dn2527-astronomers-reach-the-event-horizon.html</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>El superficie de un agujero negro.</basic:definition> + <basic:source>Oxford2003</basic:source> + </descripGrp> + <termSec> + <term>horizonte de sucesos</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>En consecuencia, aquí, cuando nos estamos + refiriendo a una «singularidad», estamos pensando en una masa con + volumen nulo rodeada de una frontera gravitacional llamada + «horizonte de sucesos», de la cual nada puede escapar. </basic:context> + <basic:source>http://www.astrocosmo.cl/h-foton/h-foton-03_08-01.htm</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>horizonte de eventos</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>InvestermSecadores de la Universidad de St. Andrews + en Escocia, afirman haber encontrado una forma de simular un + horizonte de eventos de un agujero negro – no a través de una nueva + técnica de observación cósmica, ni mediante una supercomputadora de + alta potencia … sino en el laboratorio.</basic:context> + <basic:source>http://www.cienciakanija.com/2008/02/14/horizonte-de-eventos-sintetico-de-un-agujero-negro-creado-en-un-laboratorio-del-reino-unido/</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c37"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Proton%E2%80%93proton_chain_reaction#/media/File:Fusion_in_the_Sun.svg">PP_Chain.jpg</basic:xGraphic> + <note>G-Source: http://en.wikipedia.org/wiki/File:FusionintheSun.svg</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <termSec> + <term>proton-proton chain reaction</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <basic:termType>fullForm</basic:termType> + <descripGrp> + <basic:context>The proton–proton chain reaction is one of + several fusion reactions by which stars convert hydrogen to helium, + the primary alternative being the CNO cycle. The proton–proton chain + dominates in stars the size of the Sun or smaller.</basic:context> + <basic:source>http://www.absoluteastronomy.com/topics/Proton-proton_chain_reaction</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>PP chain</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>preferredTerm-admn-sts</min:administrativeStatus> + <basic:termType>shortForm</basic:termType> + <descripGrp> + <basic:context>The primary reactions in the main branch of the + PP chain are illustrated in the following figure.</basic:context> + <basic:source>http://csep10.phys.utk.edu/astr162/lect/energy/ppchain.html</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>proton-proton reaction</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <basic:termType>variant</basic:termType> + <descripGrp> + <basic:context>The gamma rays produced in the proton-proton + reaction take one to 10 million years to work their way out from the + star's core, being scattered numerous times and losing energy as + they go, until they emerge from the surface as rays of light and + heat. Inside the Sun, about 655 million tons of hydrogen are + converted into 650 million tons of helium every second. In stars + heavier than about 2 solar masses, in which the core temperature is + more than about 18 million K, the dominant process in which energy + is produced by the fusion of hydrogen into helium is a different + reaction chain known as the carbon-nitrogen cycle. </basic:context> + <basic:source>http://www.daviddarling.info/encyclopedia/P/proton-proton_chain.html</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Un conjunto de procesos nucleares mediante los + cuales cuatro núcleos de átomos de hidrógeno se combinan para formar uno + de helio, produciendo gran cantidad de energía.</basic:definition> + <basic:source>http://www.avizora.com/publicaciones/astronomia/textos/glosario_astronomia_afines_0006.htm</basic:source> + </descripGrp> + <termSec> + <term>cadena protón-protón</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c38"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/CNO_cycle#/media/File:CNO_cycle.png">CNO_Cycle.jpg</basic:xGraphic> + <note>G-Source: http://en.wikipedia.org/wiki/File:CNO_Cycle.svg</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <termSec> + <term>carbon-nitrogen cycle</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <basic:termType>variant</basic:termType> + <descripGrp> + <basic:context>The Helium burning process are important 1) + Carbon-Nitrogen cycle at which a carbon-12 nucleus (12C) capture + proton and is converted into 13C, Nitrogen-4 and nitrogen –15. </basic:context> + <basic:source>http://www.sciencenews.org/view/generic/id/44769/title/Supernova_may_be_in_a_new_class</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>CNO cycle</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>preferredTerm-admn-sts</min:administrativeStatus> + <basic:termType>shortForm</basic:termType> + <descripGrp> + <basic:context>For stars heavier than the sun, theoretical + models show that the CNO (carbon-nitrogen-oxygen) cycle of nuclear + fusion is the dominant source of energy generation.</basic:context> + <basic:source>http://nobelprize.org/nobel_prizes/physics/articles/fusion/sun_cno.html</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>carbon-nitrogen-oxygen cycle</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <basic:termType>variant</basic:termType> + <descripGrp> + <basic:context>For stars heavier than the sun, theoretical + models show that the CNO (carbon-nitrogen-oxygen) cycle of nuclear + fusion is the dominant source of energy generation.</basic:context> + <basic:source>http://nobelprize.org/nobel_prizes/physics/articles/fusion/sun_cno.html</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>Bethe-Weizsäcker-cycle</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>Dr. von Weizsäcker is best known in science for + what is sometimes called the Bethe-Weizsäcker cycle, proposed by him + and the physicist Hans Bethe in the late 1930s as the nuclear + reactive process by which energy is generated in stars. </basic:context> + <basic:source>http://www.nytimes.com/2007/05/02/world/europe/02weizsacker.html</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>carbon cycle</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>deprecatedTerm-admn-sts</min:administrativeStatus> + <basic:termType>variant</basic:termType> + <descripGrp> + <basic:context>The main theme of the carbon cycle is the adding + of protons, but after a carbon-12 nucleus fuses with a proton to + form nitrogen-13, one of the protons decays with the emission of a + positron and a neutrino to form carbon -13.</basic:context> + <basic:source>http://hyperphysics.phy-astr.gsu.edu/HBASE/Astro/carbcyc.html</basic:source> + </descripGrp> + <note>The carbon cycle can also refer to the biogeochemical cycle by which + carbon is exchanged among the biosphere, pedosphere, geosphere, + hydrosphere, and atmosphere of the Earth.</note> + <note>N-Source: http://en.wikipedia.org/wiki/Carbon_cycle</note> + </termSec> + <termSec> + <term>CN cycle</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <basic:termType>variant</basic:termType> + <descripGrp> + <basic:context>We argue that it may be possible to exploit + neutrinos from the CN cycle and p-p chain to determine the + primordial solar core abundances of C and N at an interesting level + of precision.</basic:context> + <basic:source>http://iopscience.iop.org/0004-637X/687/1/678</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <termSec> + <term>ciclo CNO</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <basic:termType>shortForm</basic:termType> + <descripGrp> + <basic:context>Existen dos formas fundamentales en las que una + estrella fusiona hidrógeno para producir helio: la cadena + protón-protón y el ciclo CNO.</basic:context> + <basic:source>http://eltamiz.com/2007/09/06/la-vida-privada-de-las-estrellas-las-entranas-de-una-estrella/</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno-oxígeno</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>deprecatedTerm-admn-sts</min:administrativeStatus> + <basic:termType>fullForm</basic:termType> + <descripGrp> + <basic:context>No se pretende copiar los complicados ciclos de + reacciones que se dan en el interior de las estrellas, como la + cadena protón-protón o el ciclo del carbono-nitrógeno-oxígeno (esta + última más importante en las estrellas más masivas que el Sol). </basic:context> + <basic:source>http://www.zaragoza.es/ciudad/conocimiento/zivis/aplicaciones.htm</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>ciclo del carbono</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>deprecatedTerm-admn-sts</min:administrativeStatus> + <basic:termType>variant</basic:termType> + <descripGrp> + <basic:context>El ciclo del carbono comienza y acaba con un + núcleo de carbono 12 que actúa como catalizador en la producción de + un núcleo de helio a partir de núcleos de hidrógeno; también se + producen neutrinos y rayos gamma. </basic:context> + <basic:source>http://www.astromia.com/glosario/ciclocno.htm</basic:source> + </descripGrp> + <note>También este término puede referirse a la formación de las moléculas + de carbohidratos, lípidos, proteínas y ácidos nucleicos.</note> + <note>N-Source: http://es.wikipedia.org/wiki/Ciclo_del_carbono</note> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>preferredTerm-admn-sts</min:administrativeStatus> + <basic:termType>variant</basic:termType> + <descripGrp> + <basic:context>En las estrellas de gran masa, que queman su + hidrógeno mucho más rápidamente, predomina el ciclo del + carbono-nitrógeno (CN).</basic:context> + <basic:source>http://www.aavbae.net/bol17/evolucion.php</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c39"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A state of matter attained when atomic particles + are packed together as termSechtly as is physically possible, at densities + of several thousand tonnes per cubic metre.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>degeneracy</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Although Eddington raised doubts at the meeting + about the concept of relativistic degeneracy, astronomy has since + found that all white dwarfs for which masses have been measured fall + neatly below the Chandrasekhar limit without exception. Today there + are no doubts about his work on degeneracy. </basic:context> + <basic:source>http://www.tamil.net/people/andrew/subra.htm</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Estado de la materia producido cuando las + partículas atómicas tienen el mayor empaquetamiento físicamente posible, + con densidades de varios miles de toneladas por centímetro cúbico. </basic:definition> + <basic:source>http://www.emiliosilveravazquez.com/glosario.php?letra=d</basic:source> + </descripGrp> + <termSec> + <term>degeneración</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Estas estrellas son aún más densas que las + enanas blancas, y más pequeñas. Se mantienen por un proceso de + "degeneración de neutrones" o "repulsión de neutrones".</basic:context> + <basic:source>http://www.austrinus.com/index.php?option=com_content&view=article&id=157&Itemid=112</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c40"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <termSec> + <term>Oxford2003</term> + + + <note>Author[s]: Ridpath, Ian</note> + <note>Book Title: Astronomía</note> + <note>Publication Place: Spain</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c41"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>Stellar Death</min:subjectField> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>The state of degeneracy attained when the density + of matter is so high that electrons cannot be packed any closer + together.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <note>Electron degeneracy supports white dwarf stars against further + collapse.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>electron degeneracy</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>When it reaches the threshold of energy + necessary to force the combining of electrons and protons to form + neutrons, the electron degeneracy limit has been passed and the + collapse continues until it is stopped by neutron + degeneracy.</basic:context> + <basic:source>http://hyperphysics.phy-astr.gsu.edu/HBASE/Astro/pulsar.html</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>El estado de degeneración alcanzado cuando la + densidad de materia es tan grande, que los electrones no pueden + empaquetarse más.</basic:definition> + <basic:source>Oxford2003</basic:source> + </descripGrp> + <termSec> + <term>degeneración de electrones</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>Es la principal responsable de la resistencia al + colapso gravitacional de las enanas blancas (degeneración de + electrones) y de las estrellas de neutrones (degeneración de + neutrones). </basic:context> + <basic:source>http://www.emiliosilveravazquez.com/glosario.php?letra=d</basic:source> + </descripGrp> + </termSec> + <termSec> + <term>degeneración electrónica</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <min:administrativeStatus>admittedTerm-admn-sts</min:administrativeStatus> + <descripGrp> + <basic:context>Las fuerzas gravitatorias actuantes en un cuerpo + celeste masivo pueden comprimir su materia hasta un estado de + degeneración electrónica y no más, ya que el principio de exclusión + impide a dos electrones ocupar el mismo nivel de energía. </basic:context> + <basic:source>http://www.portalplanetasedna.com.ar/estrella2.htm</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c42"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-05-01</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Event_horizon#/media/File:Spacetime_lattice_analogy.svg">Event_Horizon.jpg</basic:xGraphic> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A mathematical point at which certain physical + quantities reach infinite values.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>singularity</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>A singularity means a point where some property + is infinite. For example, at the center of a black hole, according + to classical theory, the density is infinite (because a finite mass + is compressed to a zero volume). Hence it is a singularity. </basic:context> + <basic:source>http://curious.astro.cornell.edu/question.php?number=55</basic:source> + </descripGrp> + <note>Related Term: black hole, event horizon, Schwarzschild radius</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Un punto matemático en el que ciertas cantidades + físicas alcanzan valores infinitos.</basic:definition> + <basic:source>Oxford2003</basic:source> + </descripGrp> + <termSec> + <term>singularidad</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Las singularidades ocurren en el Big Bang, en + los agujeros negros y en el Big Crunch (que podría ser considerado + como una unión de agujeros negros).</basic:context> + <basic:source>http://www.astrocosmo.cl/h-foton/h-foton-03_08-01.htm</basic:source> + </descripGrp> + <note>Related Term: agujero negro, horizonte de sucesos, radio de + Schwarzschild</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c43"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Solar_mass#/media/File:Rho_Cassiopeiae_Sol_VY_Canis_Majoris.png">Solar_Mass.jpg</basic:xGraphic> + <note>G-Source: http://en.wikipedia.org/wiki/Solar_mass</note> + <note>In this graphic, the M with a subscript is the symbol for a solar mass.</note> + <note>N-Source: Jonathan Tomolonis</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A unit of mass used in stellar and galactic + astronomy, equivalent to the mass of the sun, 1.989 x 10^30 + kg.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>solar mass</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>This page now explores the fate of stars of 8 + solar masses or less.</basic:context> + <basic:source>http://outreach.atnf.csiro.au/education/senior/astrophysics/stellarevolution_deathlow.html</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Una unidad de medida utilizada en astronomía y + astrofísica para medir comparativamente la masa de las estrellas y otros + objetos astronómicos muy masivos como galaxias.</basic:definition> + <basic:source>http://es.wikipedia.org/wiki/Masa_solar</basic:source> + </descripGrp> + <termSec> + <term>masa solar</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Para una nube con la masa de nuestro Sol, el + colapso dura unos 10 millones de años, mientras que si su masa fuese + mucho más pequeña, por ejemplo un décimo de la masa solar, este + proceso podría durar hasta 800 millones de años.</basic:context> + <basic:source>http://www.tayabeixo.org/sist_solar/hipotesis/formacion_sistsolar.htm</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c44"> + <min:subjectField>General</min:subjectField> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + + <basic:xGraphic target="https://en.wikipedia.org/wiki/Triple-alpha_process#/media/File:Triple-Alpha_Process.svg">Triple-Alpha_Process.jpg</basic:xGraphic> + <note>G-Source: + http://upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Triple-Alpha_Process.svg/750px-Triple-Alpha_Process.svg.png</note> + <langSec xml:lang="en"> + + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>The chain of nuclear reactions by which carbon is + synthesized in the interiors of stars through the fusion of three helium + nuclei(alpha particles).</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>triple-alpha process</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>This small concentration of Be-8 can begin to + undergo reactions with other He-4 nuclei to produce an excited state + of the mass-12 isotope of Carbon. This excited state is unstable, + but a few of these excited Carbon nuclei emit a gamma-ray quickly + enough to become stable before they disintegrate. This extremely + improbable sequence is called the triple-alpha process because the + net effect is to combine 3 alpha particles (that is, 3 He-4 nuclei) + to form a C-12 nucleus. </basic:context> + <basic:source>http://csep10.phys.utk.edu/astr162/lect/energy/triplealph.html</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>El proceso por el cual tres núcleos de helio + (partículas alfa) se transforman en un núcleo de carbono.</basic:definition> + <basic:source>http://es.wikipedia.org/wiki/Proceso_triple-alfa</basic:source> + </descripGrp> + <termSec> + <term>proceso triple-alfa</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>También debe tenerse en cuenta una tercera + reacción de gran importancia, denominada proceso triple + alfa.</basic:context> + <basic:source>http://feinstein.com.ar/Composicion.html</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c45"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <min:subjectField>General</min:subjectField> + <basic:xGraphic target="https://en.wikipedia.org/wiki/Black_dwarf#/media/File:Black_dwarf.jpg">Black_Dwarf.jpg</basic:xGraphic> + <note>G-Source: + http://www.dorlingkindersley-uk.co.uk/static/clipart/uk/dk/sci_space/image_sci_space013.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>A degenerate star that has cooled until it is no + longer visible.</basic:definition> + <basic:source>Oxford2007</basic:source> + </descripGrp> + <termSec> + <term>black dwarf</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>Banprupt though it is, a white swarf still has a + high surface temperature when it is first formed; up to 100,000 + degrees C in some cases and it continues to radiate. Gradually it + fades, and must end up as a cold, dead black dwarf; but at the + moment no white dwarf with a surface temperature of below 3,000 + degrees C has been found, and it may be that the universe is not yet + old enough for any black dwarfs to have been formed.</basic:context> + <basic:source>Moore2003, 173</basic:source> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <basic:transactionType>origination</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <transacGrp> + <basic:transactionType>modification</basic:transactionType> + <date>2010-04-29</date> + <basic:responsibility target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</basic:responsibility> + </transacGrp> + <descripGrp> + <basic:definition>Una estrella creada cuando una enana blanca se + enfría lo suficiente como para dejar de emitir calor o luz en cantidad + significativa.</basic:definition> + <basic:source>http://spaceplace.nasa.gov/sp/kids/spitzer/signs/sign_glossary.shtml</basic:source> + </descripGrp> + <termSec> + <term>enana negra</term> + + + <min:partOfSpeech>noun</min:partOfSpeech> + <descripGrp> + <basic:context>No se conoce, todavía, la cantidad de Enanas + Negras que pueblan en realidad nuestro Universo. El tiempo estimado + para que una Enana Blanca se enfríe lo suficiente para volverse + Negra, se estima entre diez y cien mil millones de años, y nuestro + Universo no es aún lo bastante viejo, nada más que para que existan + algunas enanas blancas que se han enfriado lo suficiente para + alcanzar la etapa de enanas negras.</basic:context> + <basic:source>http://celestia.albacete.org/celestia/celestia/stars/enana12.htm</basic:source> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + </body> + <back> + <refObjectSec type="respPerson"> + <refObject id="pe324as3-9615-4d41-a9c8-30c36bffe0e6"> + <item type="fn">Tommy Tomolonis</item> + </refObject> + </refObjectSec> + </back> + </text> + +</tbx> diff --git a/reference-docs/schemas/TBX-Linguist_dialect/DCT/TBX-Linguist.nvdl b/reference-docs/schemas/TBX-Linguist_dialect/DCT/TBX-Linguist.nvdl new file mode 100644 index 0000000..8cf6a45 --- /dev/null +++ b/reference-docs/schemas/TBX-Linguist_dialect/DCT/TBX-Linguist.nvdl @@ -0,0 +1,41 @@ +<?xml version="1.0" encoding="UTF-8"?> +<rules xmlns="http://purl.oclc.org/dsdl/nvdl/ns/structure/1.0" + xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0" startMode="core"> + <mode name="core"> + <namespace ns="urn:iso:std:iso:30042:ed-2"> + <validate schema="https://raw.githubusercontent.com/LTAC-Global/TBX_Core_RNG/master/TBXcoreStructV03.rng" useMode="RNG"/> + <validate schema="https://raw.githubusercontent.com/LTAC-Global/TBX-Linguist_dialect/master/DCT/TBX-Linguist_DCT.sch" useMode="SCH"/> + <validate schema="https://raw.githubusercontent.com/LTAC-Global/TBX_linguist_module/master/Linguist.sch" useMode="SCH"/> + <validate schema="https://raw.githubusercontent.com/LTAC-Global/TBX_basic_module/master/Basic.sch" useMode="SCH"/> + <validate schema="https://raw.githubusercontent.com/LTAC-Global/TBX_min_module/master/Min.sch" useMode="SCH"/> + </namespace> + <anyNamespace> + <reject/> + </anyNamespace> + </mode> + <mode name="RNG"> + <namespace ns="http://www.tbxinfo.net/ns/min"> + <validate schema="https://raw.githubusercontent.com/LTAC-Global/TBX_min_module/master/Min.rng"/> + <attach/> + </namespace> + <namespace ns="http://www.tbxinfo.net/ns/basic"> + <validate schema="https://raw.githubusercontent.com/LTAC-Global/TBX_basic_module/master/Basic.rng"/> + <attach/> + </namespace> + <namespace ns="http://www.tbxinfo.net/ns/linguist"> + <validate schema="https://raw.githubusercontent.com/LTAC-Global/TBX_linguist_module/master/Linguist.rng"/> + <attach/> + </namespace> + </mode> + <mode name="SCH"> + <namespace ns="http://www.tbxinfo.net/ns/min"> + <attach/> + </namespace> + <namespace ns="http://www.tbxinfo.net/ns/basic"> + <attach/> + </namespace> + <namespace ns="http://www.tbxinfo.net/ns/linguist"> + <attach/> + </namespace> + </mode> +</rules> \ No newline at end of file diff --git a/reference-docs/schemas/TBX-Linguist_dialect/DCT/TBX-Linguist_DCT.sch b/reference-docs/schemas/TBX-Linguist_dialect/DCT/TBX-Linguist_DCT.sch new file mode 100644 index 0000000..24c4142 --- /dev/null +++ b/reference-docs/schemas/TBX-Linguist_dialect/DCT/TBX-Linguist_DCT.sch @@ -0,0 +1,48 @@ +<?xml version="1.0" encoding="UTF-8"?> +<schema xmlns="http://purl.oclc.org/dsdl/schematron" queryBinding="xslt2" + xmlns:sqf="http://www.schematron-quickfix.com/validator/process"> + <ns uri="urn:iso:std:iso:30042:ed-2" prefix="tbx" /> + + <pattern id="coreEnforecement"> + <rule context="tbx:termNote"> + <assert test="parent::tbx:termSec or parent::tbx:termNoteGrp/parent::tbx:termSec">Any termNote is only allowed at the termSec level.</assert> + </rule> + <rule context="tbx:*[@metatype='termNote']"> + <assert test="parent::tbx:termSec or parent::tbx:termNoteGrp/parent::tbx:termSec">Any termNote is only allowed at the termSec level.</assert> + </rule> + <rule context="*[@target]"> + <assert test="matches(@target,'https?://.+') or @target = //*/@id">ID must be IDREF for internal references or URI following HTTP protocol for external references.</assert> + </rule> + </pattern> + + <pattern id="XLIFF.inlineConstraints"> + <rule context="tbx:sc[following-sibling::tbx:ec]"> + <assert test="@isolated='no' or not(@isolated)">@isolated must be 'no' if <sc/> or <ec/> has its corresponding <sc/>/<ec/> in the same note text and @startRef must be used for <ec></assert> + </rule> + <rule context="tbx:ec[preceding-sibling::tbx:sc]"> + <assert test="@isolated='no' or not(@isolated)">@isolated must be 'no' if <sc/> or <ec/> has its corresponding <sc/>/<ec/> in the same note text and @startRef must be used for <ec></assert> + <assert test="@startRef">@starRef is required for <ec> if it is in the same note text as its corresponding <sc></assert> + <!--<assert test="not(@dir)">@dir only permitted when @isolated is 'yes'.</assert>--><!--@dir IS NOT CURRENTLY USED IN TBX--> + </rule> + <rule context="tbx:sc[not(following-sibling::tbx:ec)]"> + <assert test="@isolated='yes' or not(@isolated)">@isolated must be 'yes' if <sc/> or <ec/> does not have its corresponding <sc/>/<sc/> in the same note text</assert> + </rule> + <rule context="tbx:ec[not(preceding-sibling::tbx:sc)]"> + <assert test="@isolated='yes' or not(@isolated)">@isolated must be 'yes' if <sc/> or <ec/> does not have its corresponding <sc/>/<sc/> in the same note text</assert> + <assert test="@id">@id is REQUIRED when @isolated is or should be 'yes'.</assert> + </rule> + <rule context="tbx:ec[@isolated='yes']"> + <assert test="@id != ''">ID is required if @isolated is 'yes'.</assert> + </rule> + </pattern> + + <pattern id="dialectEnforcement"> + <rule context="tbx:tbx"> + <assert test="attribute::type='TBX-Linguist'">The name of this dialect should be TBX-Linguist</assert> + <assert test="attribute::style='dct'">The style of this dialect should be declared as 'dct'</assert> + </rule> + <rule context="tbx:*[@type]"> + <assert test="not(matches(.,'|.')) or .. is root() or ancestor::tbx:back or ancestor::tbx:tbxHeader">DCA style elements are not permitted in DCT style TBX.</assert> + </rule> + </pattern> +</schema> \ No newline at end of file diff --git a/reference-docs/schemas/TBX-Linguist_dialect/TBX-Linguist Definition.pdf b/reference-docs/schemas/TBX-Linguist_dialect/TBX-Linguist Definition.pdf new file mode 100644 index 0000000..9d2dc4c Binary files /dev/null and b/reference-docs/schemas/TBX-Linguist_dialect/TBX-Linguist Definition.pdf differ diff --git a/reference-docs/schemas/TBX-Min_dialect/DCA/TBX-Min_DCA.sch b/reference-docs/schemas/TBX-Min_dialect/DCA/TBX-Min_DCA.sch new file mode 100644 index 0000000..26239cd --- /dev/null +++ b/reference-docs/schemas/TBX-Min_dialect/DCA/TBX-Min_DCA.sch @@ -0,0 +1,82 @@ +<?xml version="1.0" encoding="utf-8"?> +<schema queryBinding="xslt2" xmlns:sqf="http://www.schematron-quickfix.com/validator/process" xmlns="http://purl.oclc.org/dsdl/schematron"> + <ns uri="urn:iso:std:iso:30042:ed-2" prefix="tbx" /> + <pattern id="coreEnforcement"> + <rule context="tbx:termNote"> + <assert test="parent::tbx:termSec or parent::tbx:termNoteGrp/parent::tbx:termSec">Any termNote is only allowed at the termSec level.</assert> + </rule> + <rule context="tbx:*[@type]"> + <assert test="@type != ''">Data category must be declared. If no permitted data categories are listed in the grammar schema, blank values are also not allowed.</assert> + </rule> + <rule context="*[@target]"> + <assert test="matches(@target,'https?://.+') or @target = //*/@id">ID must be IDREF for internal references or URI following HTTP protocol for external references.</assert> + </rule> + </pattern> + <pattern id="XLIFF.inlineConstraints"> + <rule context="tbx:sc[following-sibling::tbx:ec]"> + <assert test="@isolated='no' or not(@isolated)">@isolated must be 'no' if <sc/> or <ec/> has its corresponding <sc/>/<ec/> in the same note text and @startRef must be used for <ec></assert> + </rule> + <rule context="tbx:ec[preceding-sibling::tbx:sc]"> + <assert test="@isolated='no' or not(@isolated)">@isolated must be 'no' if <sc/> or <ec/> has its corresponding <sc/>/<ec/> in the same note text and @startRef must be used for <ec></assert> + <assert test="@startRef">@starRef is required for <ec> if it is in the same note text as its corresponding <sc></assert> + <!--<assert test="not(@dir)">@dir only permitted when @isolated is 'yes'.</assert>--> + <!--@dir IS NOT CURRENTLY USED IN TBX--> + </rule> + <rule context="tbx:sc[not(following-sibling::tbx:ec)]"> + <assert test="@isolated='yes' or not(@isolated)">@isolated must be 'yes' if <sc/> or <ec/> does not have its corresponding <sc/>/<sc/> in the same note text.</assert> + </rule> + <rule context="tbx:ec[not(preceding-sibling::tbx:sc)]"> + <assert test="@isolated='yes' or not(@isolated)">@isolated must be 'yes' if <sc/> or <ec/> does not have its corresponding <sc/>/<sc/> in the same note text.</assert> + <assert test="@id">@id is REQUIRED when @isolated is or should be 'yes'.</assert> + </rule> + <rule context="tbx:ec[@isolated='yes']"> + <assert test="@id != ''">ID is required if @isolated is 'yes'.</assert> + </rule> + </pattern> + <pattern id="dialectEnforcement"> + <rule context="tbx:tbx"> + <assert test="attribute::type='TBX-Min'">The name of this dialect should be TBX-Min.</assert> + <assert test="attribute::style='dca'">The style of this dialect should be declared as 'dca'.</assert> + </rule> + <rule context="*[not(namespace-uri() = 'urn:iso:std:iso:30042:ed-2')]"> + <assert test="false()">DCT style elements are not permitted in DCA style TBX.</assert> + </rule> + <!-- Data Category Types --> + <rule context="tbx:admin/@type"> + <assert test=".='customerSubset'">Permitted type value(s): customerSubset</assert> + </rule> + <rule context="tbx:descrip/@type"> + <assert test=".='subjectField'">Permitted type value(s): subjectField</assert> + </rule> + <rule context="tbx:termNote/@type"> + <assert test=".='administrativeStatus' or .='partOfSpeech'">Permitted type value(s): administrativeStatus, partOfSpeech</assert> + </rule> + <rule context="tbx:xref/@type"> + <assert test=".='externalCrossReference'">Permitted type value(s): externalCrossReference</assert> + </rule> + </pattern> + <!-- min module rules --> + <pattern id="module.min.admin"> + <rule context="tbx:admin[@type='customerSubset']"> + <assert test="parent::tbx:conceptEntry or parent::tbx:*[contains(./local-name(),'Grp')][not(./local-name() = 'transacGrp')]/parent::tbx:conceptEntry or parent::tbx:termSec or parent::tbx:*[contains(./local-name(),'Grp')][not(./local-name() = 'transacGrp')]/parent::tbx:termSec">/customerSubset/ may only appear at level(s): conceptEntry, termSec</assert> + </rule> + </pattern> + <pattern id="module.min.descrip"> + <rule context="tbx:descrip[@type='subjectField']"> + <assert test="parent::tbx:conceptEntry or parent::tbx:descripGrp/parent::tbx:conceptEntry">/subjectField/ may only appear at level(s): conceptEntry</assert> + </rule> + </pattern> + <pattern id="module.min.termNote"> + <rule context="tbx:termNote[@type='administrativeStatus']"> + <assert test=".='admittedTerm-admn-sts' or .='deprecatedTerm-admn-sts' or .='supersededTerm-admn-sts' or .='preferredTerm-admn-sts'">/administrativeStatus/ type may be: 'admittedTerm-admn-sts' or 'deprecatedTerm-admn-sts' or 'supersededTerm-admn-sts' or 'preferredTerm-admn-sts'</assert> + </rule> + <rule context="tbx:termNote[@type='partOfSpeech']"> + <assert test=".='adjective' or .='noun' or .='other' or .='verb' or .='adverb'">/partOfSpeech/ type may be: 'adjective' or 'noun' or 'other' or 'verb' or 'adverb'</assert> + </rule> + </pattern> + <pattern id="module.min.xref"> + <rule context="tbx:xref[@type='externalCrossReference']"> + <assert test="parent::tbx:conceptEntry or parent::tbx:langSec or parent::tbx:termSec">/externalCrossReference/ may only appear at level(s): conceptEntry, langSec, termSec</assert> + </rule> + </pattern> +</schema> \ No newline at end of file diff --git a/reference-docs/schemas/TBX-Min_dialect/DCT/TBX-Min.nvdl b/reference-docs/schemas/TBX-Min_dialect/DCT/TBX-Min.nvdl new file mode 100644 index 0000000..3792de5 --- /dev/null +++ b/reference-docs/schemas/TBX-Min_dialect/DCT/TBX-Min.nvdl @@ -0,0 +1,25 @@ +<?xml version="1.0" encoding="UTF-8"?> +<rules xmlns="http://purl.oclc.org/dsdl/nvdl/ns/structure/1.0" + xmlns:a="http://relaxng.org/ns/compatibility/annotations/1.0" startMode="core"> + <mode name="core"> + <namespace ns="urn:iso:std:iso:30042:ed-2"> + <validate schema="https://raw.githubusercontent.com/LTAC-Global/TBX_Core_RNG/master/TBXcoreStructV03.rng" useMode="RNG"/> + <validate schema="https://raw.githubusercontent.com/LTAC-Global/TBX-Min_dialect/master/DCT/TBX-Min_DCT.sch" useMode="SCH"/> + <validate schema="https://raw.githubusercontent.com/LTAC-Global/TBX_min_module/master/Min.sch" useMode="SCH"/> + </namespace> + <anyNamespace> + <reject/> + </anyNamespace> + </mode> + <mode name="RNG"> + <namespace ns="http://www.tbxinfo.net/ns/min"> + <validate schema="https://raw.githubusercontent.com/LTAC-Global/TBX_min_module/master/Min.rng"/> + <attach/> + </namespace> + </mode> + <mode name="SCH"> + <namespace ns="http://www.tbxinfo.net/ns/min"> + <attach/> + </namespace> + </mode> +</rules> \ No newline at end of file diff --git a/reference-docs/schemas/TBX-Min_dialect/DCT/TBX-Min_DCT.sch b/reference-docs/schemas/TBX-Min_dialect/DCT/TBX-Min_DCT.sch new file mode 100644 index 0000000..67c0e85 --- /dev/null +++ b/reference-docs/schemas/TBX-Min_dialect/DCT/TBX-Min_DCT.sch @@ -0,0 +1,48 @@ +<?xml version="1.0" encoding="UTF-8"?> +<schema xmlns="http://purl.oclc.org/dsdl/schematron" queryBinding="xslt2" + xmlns:sqf="http://www.schematron-quickfix.com/validator/process"> + <ns uri="urn:iso:std:iso:30042:ed-2" prefix="tbx" /> + + <pattern id="coreEnforecement"> + <rule context="tbx:termNote"> + <assert test="parent::tbx:termSec or parent::tbx:termNoteGrp/parent::tbx:termSec">Any termNote is only allowed at the termSec level.</assert> + </rule> + <rule context="tbx:*[@metatype='termNote']"> + <assert test="parent::tbx:termSec or parent::tbx:termNoteGrp/parent::tbx:termSec">Any termNote is only allowed at the termSec level.</assert> + </rule> + <rule context="*[@target]"> + <assert test="matches(@target,'https?://.+') or @target = //*/@id">ID must be IDREF for internal references or URI following HTTP protocol for external references.</assert> + </rule> + </pattern> + + <pattern id="XLIFF.inlineConstraints"> + <rule context="tbx:sc[following-sibling::tbx:ec]"> + <assert test="@isolated='no' or not(@isolated)">@isolated must be 'no' if <sc/> or <ec/> has its corresponding <sc/>/<ec/> in the same note text and @startRef must be used for <ec></assert> + </rule> + <rule context="tbx:ec[preceding-sibling::tbx:sc]"> + <assert test="@isolated='no' or not(@isolated)">@isolated must be 'no' if <sc/> or <ec/> has its corresponding <sc/>/<ec/> in the same note text and @startRef must be used for <ec></assert> + <assert test="@startRef">@starRef is required for <ec> if it is in the same note text as its corresponding <sc></assert> + <!--<assert test="not(@dir)">@dir only permitted when @isolated is 'yes'.</assert>--><!--@dir IS NOT CURRENTLY USED IN TBX--> + </rule> + <rule context="tbx:sc[not(following-sibling::tbx:ec)]"> + <assert test="@isolated='yes' or not(@isolated)">@isolated must be 'yes' if <sc/> or <ec/> does not have its corresponding <sc/>/<sc/> in the same note text</assert> + </rule> + <rule context="tbx:ec[not(preceding-sibling::tbx:sc)]"> + <assert test="@isolated='yes' or not(@isolated)">@isolated must be 'yes' if <sc/> or <ec/> does not have its corresponding <sc/>/<sc/> in the same note text</assert> + <assert test="@id">@id is REQUIRED when @isolated is or should be 'yes'.</assert> + </rule> + <rule context="tbx:ec[@isolated='yes']"> + <assert test="@id != ''">ID is required if @isolated is 'yes'.</assert> + </rule> + </pattern> + + <pattern id="dialectEnforcement"> + <rule context="tbx:tbx"> + <assert test="attribute::type='TBX-Min'">The name of this dialect should be TBX-Min</assert> + <assert test="attribute::style='dct'">The style of this dialect should be declared as 'dct'</assert> + </rule> + <rule context="tbx:*[@type]"> + <assert test="not(matches(.,'|.')) or .. is root() or ancestor::tbx:back or ancestor::tbx:tbxHeader">DCA style elements are not permitted in DCT style TBX.</assert> + </rule> + </pattern> +</schema> \ No newline at end of file diff --git a/reference-docs/schemas/TBX-Min_dialect/TBX-Min Definition.pdf b/reference-docs/schemas/TBX-Min_dialect/TBX-Min Definition.pdf new file mode 100644 index 0000000..f2ee949 Binary files /dev/null and b/reference-docs/schemas/TBX-Min_dialect/TBX-Min Definition.pdf differ diff --git a/reference-docs/schemas/TBX_linguist_module/Linguist Module Definition.pdf b/reference-docs/schemas/TBX_linguist_module/Linguist Module Definition.pdf new file mode 100644 index 0000000..471eab2 Binary files /dev/null and b/reference-docs/schemas/TBX_linguist_module/Linguist Module Definition.pdf differ diff --git a/reference-docs/schemas/TBX_linguist_module/Linguist.rng b/reference-docs/schemas/TBX_linguist_module/Linguist.rng new file mode 100644 index 0000000..bea8c33 --- /dev/null +++ b/reference-docs/schemas/TBX_linguist_module/Linguist.rng @@ -0,0 +1,93 @@ +<?xml version="1.0" encoding="utf-8"?> +<grammar xmlns="http://relaxng.org/ns/structure/1.0" xmlns:xlink="http://www.w3.org/1999/xlink" + xmlns:teix="http://www.tei-c.org/ns/Examples" + datatypeLibrary="http://www.w3.org/2001/XMLSchema-datatypes" + ns="http://www.tbxinfo.net/ns/linguist"> + + <!-- optional metaType attribute --> + <define name="metaType"> + <optional> + <attribute name="metaType"> + <choice> + <value>admin</value> + <value>adminNote</value> + <value>descrip</value> + <value>descripNote</value> + <value>ref</value> + <value>termNote</value> + <value>transac</value> + <value>transacNote</value> + <value>xref</value> + </choice> + </attribute> + </optional> + </define> + + <!-- shared attributes --> + <define name="attribute.target.internal"> + <attribute name="target"> + <data type="IDREF"/> + </attribute> + </define> + <define name="attribute.target.external"> + <attribute name="target"> + <data type="anyURI"> + <param name="pattern">https?://.+</param> + </data> + </attribute> + </define> + + + <define name="module.admin"> + <choice> + <element name="reading"> + <text/> + </element> + </choice> + </define> + + <define name="module.adminNote"> + <choice> + <element name="readingNote"> + <text/> + </element> + </choice> + </define> + + <!-- termNote classified elements --> + <define name="module.termNote"> + <choice> + <element name="grammaticalNumber"> + <choice> + <value>singular</value> + <value>plural</value> + <value>dual</value> + <value>mass</value> + <value>otherNumber</value> + </choice> + </element> + <element name="register"> + <choice> + <value>colloquialRegister</value> + <value>neutralRegister</value> + <value>technicalRegister</value> + <value>in-houseRegister</value> + <value>bench-levelRegister</value> + <value>slangRegister</value> + <value>vulgarRegister</value> + </choice> + </element> + <element name="transferComment"> + <text/> + </element> + </choice> + </define> + + <start> + <choice> + <ref name="module.admin"/> + <ref name="module.adminNote"/> + <ref name="module.termNote"/> + </choice> + </start> +</grammar> diff --git a/reference-docs/schemas/TBX_linguist_module/Linguist.sch b/reference-docs/schemas/TBX_linguist_module/Linguist.sch new file mode 100644 index 0000000..bbe879c --- /dev/null +++ b/reference-docs/schemas/TBX_linguist_module/Linguist.sch @@ -0,0 +1,33 @@ +<?xml version="1.0" encoding="UTF-8"?> +<schema xmlns="http://purl.oclc.org/dsdl/schematron" queryBinding="xslt2" + xmlns:sqf="http://www.schematron-quickfix.com/validator/process"> + <ns uri="urn:iso:std:iso:30042:ed-2" prefix="tbx" /> + <ns uri="http://www.tbxinfo.net/ns/linguist" prefix="ling" /> + <ns uri="http://www.w3.org/2001/XMLSchema" prefix="xs" /> + + <!-- Linguist Module Rules --> + <pattern id="module.linguist.admin"> + <rule context="ling:reading"> + <assert test="parent::tbx:termSec or parent::tbx:adminGrp/parent::tbx:termSec">Reading must be at the term level.</assert> + </rule> + </pattern> + + <pattern id="module.linguist.adminNote"> + <rule context="ling:readingNote"> + <assert test="parent::tbx:adminGrp/parent::tbx:termSec">readingNote may only be found at the termSec level inside an adminGrp.</assert> + </rule> + </pattern> + + <pattern id="module.linguist.termNote"> + <rule context="ling:grammaticalNumber"> + <assert test="parent::tbx:termSec or parent::tbx:termNoteGrp/parent::tbx:termSec">termNote elements must not occur outside the termSec level.</assert> + </rule> + <rule context="ling:register"> <!-- note: this is also known as /usageRegister/ and should be converted to /register/ here --> + <assert test="parent::tbx:termSec or parent::tbx:termNoteGrp/parent::tbx:termSec">termNote elements must not occur outside the termSec level.</assert> + </rule> + <rule context="ling:transferComment"> + <assert test="parent::tbx:termSec or parent::tbx:termNoteGrp/parent::tbx:termSec">termNote elements must not occur outside the termSec level.</assert> + </rule> + </pattern> + +</schema> \ No newline at end of file diff --git a/reference-docs/schemas/TBX_linguist_module/Linguist.tbxmd b/reference-docs/schemas/TBX_linguist_module/Linguist.tbxmd new file mode 100644 index 0000000..1b1c6ad --- /dev/null +++ b/reference-docs/schemas/TBX_linguist_module/Linguist.tbxmd @@ -0,0 +1,47 @@ +<?xml version="1.0" encoding="UTF-8"?> +<?xml-model href="https://raw.githubusercontent.com/LTAC-Global/TBX_module_description_xml/master/tbxmd.rng" type="application/xml" schematypens="http://relaxng.org/ns/structure/1.0"?> +<tbxmd module="linguist" ns="http://www.tbxinfo.net/ns/linguist"><!-- ns is only applicable to DCT style TBX --> + <header> + <title>Description of the Linguist data category module for TBX + The Linguist module is a simple data category module created for moderate need terminology data models. + + + + + + singular + plural + dual + mass + otherNumber + + + + + termSec + + + + + + termSec + + + + + + colloquialRegister + neutralRegister + technicalRegister + in-houseRegister + bench-levelRegister + slangRegister + vulgarRegister + + + + + + + \ No newline at end of file diff --git a/reference-docs/schemas/TBX_module_description_xml/TBX Module Description.pdf b/reference-docs/schemas/TBX_module_description_xml/TBX Module Description.pdf new file mode 100644 index 0000000..2fa3245 Binary files /dev/null and b/reference-docs/schemas/TBX_module_description_xml/TBX Module Description.pdf differ diff --git a/reference-docs/schemas/TBX_module_description_xml/tbxmd.rng b/reference-docs/schemas/TBX_module_description_xml/tbxmd.rng new file mode 100644 index 0000000..7e59f2d --- /dev/null +++ b/reference-docs/schemas/TBX_module_description_xml/tbxmd.rng @@ -0,0 +1,192 @@ + + + + + + If the permitted contents of a data category are picklist values, they + will be placed here in <value> tags. Any other data category must select from + one of the 4 permitted text datatypes as described in Section 9.5 of ISO + 30042. + + + + + + + + + + + + + + + + + + + + The values permitted here are found in ISO 30042. + + string + basicText + noteText + + + + + + picklist + + + + + : This element contains the collection of permitted data categories in + the module. + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + This element is used to provide all necessary information to describe a + single data category. + + + + + + + This is the name of the data category + + + + This is the URI pointing to the source of the data category. For + standard data categories found on www.datcatinfo.net, this is the + PID. + + + + + + A description of the module being described + + + + + + + Container for header information. + + + + + + + + + + conceptEntry + langSec + termSec + + + + + + The levels in which the data category may occur. + + + + + + + + The root element of an MDF file. + + This is the name of the module + + + + This is the namespace of the module (for use in DCT style TBX + files) + + + + + + + + + + bibl + binaryData + conceptSysDescrip + element + entry + external + respPerson + term + thesaurusDescrip + + + + + + + + + + This element is used to provide a more descriptive name for a module, + in contrast to the simple name given in the @module attribute of + <mdf>> + + + + + + A <value> element contains a specific allowed instance of text + for a given data category. For example, if the data category is /partOfSpeech/, one + of the <value> elements in the <contents> section would be: + <value>noun</value> + + + + + + + + diff --git a/reference-docs/schemas/TBX_termComp_module/TermComp-namespace.rng b/reference-docs/schemas/TBX_termComp_module/TermComp-namespace.rng new file mode 100644 index 0000000..2dec87c --- /dev/null +++ b/reference-docs/schemas/TBX_termComp_module/TermComp-namespace.rng @@ -0,0 +1,156 @@ + + + + + + + + + + + + + + + + + + + + + + + + + Indicates + the language of the element content. The allowed values are found in IETF RFC 4646 or + its successor. This attribute is optional for elements that use this attribute class. + For a description, see the information at the tbx element. + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + Indicates + the type of the termCompSec, such as hyphenation. The value indicates on what basis + the term components were identified, such as by hyphenation parts or by + syllables. + + hyphenation + (Hyphenation) The termComp elements contain the parts of a term as it would be + hyphenated, such as at the end of a line, according to a given set of + rules. + lemma + (Lemma) The termComp elements contain the base form of the term or of the + individual words that it comprises. A base form of a word or term, sometimes + called a lemma, is the form that is used as the formal dictionary entry for the + term. For nouns, the base form is frequently the nominative singular form (in + languages that show variation by case). For adjectives it is the positive form of + the adjective, as opposed to the comparative, and in some languages it is + uninflected, whereas in others it is the masculine singular. For verbs, it is + generally the infinitive. + morphologicalElement + (Morphological element) The termComp elements contain the individual morphemes + that comprise the term. . + syllabification + (Syllabification) The termComp elements contain the individual syllables that + comprise the term. + termElement + (Term + element) The termComp elements contain any other logically significant portion of + the term. + + + + + + + Indicates + the type of the termCompSec, such as hyphenation. The value indicates on what basis the + term components were identified, such as by hyphenation parts or by + syllables. + + For an integrated schema for use in non-namespace environments (DCA style), + replace <text/> with the allowed values of the "type" attribute. + + + + + + + + + + + + + + + + + + + + + + + \ No newline at end of file diff --git a/spec/tbx/admin_spec.rb b/spec/tbx/admin_spec.rb new file mode 100644 index 0000000..503d94d --- /dev/null +++ b/spec/tbx/admin_spec.rb @@ -0,0 +1,64 @@ +# frozen_string_literal: true + +require "spec_helper" + +RSpec.describe Tbx::Admin do + describe "TYPES" do + it "composes types from Min, Basic, and Linguist modules" do + expected = %w[customerSubset projectSubset source reading] + expect(described_class::TYPES.values.sort).to eq(expected.sort) + end + + it "defines customerSubset from Min" do + expect(described_class::TYPES[:customer_subset]).to eq("customerSubset") + end + + it "defines projectSubset from Basic" do + expect(described_class::TYPES[:project_subset]).to eq("projectSubset") + end + + it "defines source from Basic" do + expect(described_class::TYPES[:source]).to eq("source") + end + + it "defines reading from Linguist" do + expect(described_class::TYPES[:reading]).to eq("reading") + end + end + + describe "creation" do + it "creates an admin with type and content" do + admin = described_class.new( + type: "source", + content: ["ISO 30042:2019"], + ) + expect(admin.type).to eq("source") + expect(admin.content).to eq(["ISO 30042:2019"]) + end + end + + describe "XML round-trip" do + it "round-trips an admin element through XML" do + admin = described_class.new( + type: "customerSubset", + content: ["engineering"], + ) + xml = admin.to_xml + parsed = described_class.from_xml(xml) + expect(parsed.type).to eq("customerSubset") + expect(parsed.content.join).to eq("engineering") + end + + it "round-trips an admin with inline hi element" do + admin = described_class.new( + type: "source", + content: ["Text from "], + hi: [Tbx::Hi.new(content: ["author"])], + ) + xml = admin.to_xml + parsed = described_class.from_xml(xml) + expect(parsed.type).to eq("source") + expect(parsed.hi.length).to eq(1) + end + end +end diff --git a/spec/tbx/data_element_spec.rb b/spec/tbx/data_element_spec.rb new file mode 100644 index 0000000..fa149ac --- /dev/null +++ b/spec/tbx/data_element_spec.rb @@ -0,0 +1,93 @@ +# frozen_string_literal: true + +require "spec_helper" + +RSpec.describe Tbx::DataElement do + describe "classes that include DataElement + InlineContent" do + [Tbx::Admin, Tbx::Descrip, Tbx::TermNote].each do |klass| + describe klass do + it "has id attribute" do + instance = klass.new + expect(instance).to respond_to(:id) + end + + it "has lang attribute" do + instance = klass.new + expect(instance).to respond_to(:lang) + end + + it "has target attribute" do + instance = klass.new + expect(instance).to respond_to(:target) + end + + it "has datatype attribute" do + instance = klass.new + expect(instance).to respond_to(:datatype) + end + + it "has type attribute" do + instance = klass.new + expect(instance).to respond_to(:type) + end + + it "has content attribute" do + instance = klass.new + expect(instance).to respond_to(:content) + end + + it "has inline hi attribute" do + instance = klass.new + expect(instance).to respond_to(:hi) + end + + it "has inline ec attribute" do + instance = klass.new + expect(instance).to respond_to(:ec) + end + + it "has inline foreign attribute" do + instance = klass.new + expect(instance).to respond_to(:foreign) + end + + it "has inline ph attribute" do + instance = klass.new + expect(instance).to respond_to(:ph) + end + + it "has inline sc attribute" do + instance = klass.new + expect(instance).to respond_to(:sc) + end + end + end + end + + describe "classes that include DataElement only (no InlineContent)" do + [Tbx::AdminNote, Tbx::DescripNote, Tbx::TransacNote, Tbx::Transac, + Tbx::Ref].each do |klass| + describe klass do + it "has id attribute" do + instance = klass.new + expect(instance).to respond_to(:id) + end + + it "has type attribute" do + instance = klass.new + expect(instance).to respond_to(:type) + end + + it "has content attribute" do + instance = klass.new + expect(instance).to respond_to(:content) + end + + it "does NOT have inline hi attribute" do + instance = klass.new + expect(instance).not_to respond_to(:hi) + end + end + end + end +end diff --git a/spec/tbx/descrip_spec.rb b/spec/tbx/descrip_spec.rb new file mode 100644 index 0000000..4c7bbaa --- /dev/null +++ b/spec/tbx/descrip_spec.rb @@ -0,0 +1,48 @@ +# frozen_string_literal: true + +require "spec_helper" + +RSpec.describe Tbx::Descrip do + describe "TYPES" do + it "composes types from Min and Basic modules" do + expected = %w[subjectField context definition] + expect(described_class::TYPES.values.sort).to eq(expected.sort) + end + + it "defines subjectField from Min" do + expect(described_class::TYPES[:subject_field]).to eq("subjectField") + end + + it "defines context from Basic" do + expect(described_class::TYPES[:context]).to eq("context") + end + + it "defines definition from Basic" do + expect(described_class::TYPES[:definition]).to eq("definition") + end + end + + describe "creation" do + it "creates a definition descrip" do + descrip = described_class.new( + type: "definition", + content: ["A term for testing purposes."], + ) + expect(descrip.type).to eq("definition") + expect(descrip.content).to eq(["A term for testing purposes."]) + end + end + + describe "XML round-trip" do + it "round-trips a descrip through XML" do + descrip = described_class.new( + type: "subjectField", + content: ["astronomy"], + ) + xml = descrip.to_xml + parsed = described_class.from_xml(xml) + expect(parsed.type).to eq("subjectField") + expect(parsed.content.join).to eq("astronomy") + end + end +end diff --git a/spec/tbx/hi_spec.rb b/spec/tbx/hi_spec.rb new file mode 100644 index 0000000..b8d0af3 --- /dev/null +++ b/spec/tbx/hi_spec.rb @@ -0,0 +1,66 @@ +# frozen_string_literal: true + +require "spec_helper" + +RSpec.describe Tbx::Hi do + describe "TYPES" do + it "defines all 7 core RNG hi types" do + expected = %w[entailedTerm hotkey italics bold superscript subscript math] + expect(described_class::TYPES.values.sort).to eq(expected.sort) + end + + it "defines entailedTerm type" do + expect(described_class::TYPES[:entailed_term]).to eq("entailedTerm") + end + + it "defines hotkey type" do + expect(described_class::TYPES[:hotkey]).to eq("hotkey") + end + + it "defines italics type" do + expect(described_class::TYPES[:italics]).to eq("italics") + end + + it "defines bold type" do + expect(described_class::TYPES[:bold]).to eq("bold") + end + + it "defines superscript type" do + expect(described_class::TYPES[:superscript]).to eq("superscript") + end + + it "defines subscript type" do + expect(described_class::TYPES[:subscript]).to eq("subscript") + end + + it "defines math type" do + expect(described_class::TYPES[:math]).to eq("math") + end + end + + describe "creation" do + it "creates an entailedTerm hi with target" do + hi = described_class.new( + type: "entailedTerm", + target: "c1", + content: ["related term"], + ) + expect(hi.type).to eq("entailedTerm") + expect(hi.target).to eq("c1") + expect(hi.content).to eq(["related term"]) + end + end + + describe "XML round-trip" do + it "round-trips a hi element through XML" do + hi = described_class.new( + type: "italics", + content: ["emphasized text"], + ) + xml = hi.to_xml + parsed = described_class.from_xml(xml) + expect(parsed.type).to eq("italics") + expect(parsed.content.join).to eq("emphasized text") + end + end +end diff --git a/spec/tbx/modules/basic_spec.rb b/spec/tbx/modules/basic_spec.rb new file mode 100644 index 0000000..c380c5f --- /dev/null +++ b/spec/tbx/modules/basic_spec.rb @@ -0,0 +1,89 @@ +# frozen_string_literal: true + +require "spec_helper" + +RSpec.describe Tbx::Modules::Basic do + describe "ADMIN_TYPES" do + it "contains projectSubset and source" do + expect(described_class::ADMIN_TYPES[:project_subset]) + .to eq("projectSubset") + expect(described_class::ADMIN_TYPES[:source]).to eq("source") + end + end + + describe "DESCRIP_TYPES" do + it "contains context and definition" do + expect(described_class::DESCRIP_TYPES[:context]).to eq("context") + expect(described_class::DESCRIP_TYPES[:definition]).to eq("definition") + end + end + + describe "TERM_NOTE_TYPES" do + it "contains geographicalUsage, grammaticalGender, termLocation, termType" \ + do + expect(described_class::TERM_NOTE_TYPES[:geographical_usage]) + .to eq("geographicalUsage") + expect(described_class::TERM_NOTE_TYPES[:grammatical_gender]) + .to eq("grammaticalGender") + expect(described_class::TERM_NOTE_TYPES[:term_location]) + .to eq("termLocation") + expect(described_class::TERM_NOTE_TYPES[:term_type]).to eq("termType") + end + end + + describe "TERM_NOTE_VALUES" do + it "defines grammaticalGender picklist values" do + vals = described_class::TERM_NOTE_VALUES[:grammatical_gender] + expect(vals.values.sort).to eq(%w[masculine feminine neuter other].sort) + end + + it "defines termLocation picklist with 18 values" do + vals = described_class::TERM_NOTE_VALUES[:term_location] + expect(vals.length).to eq(18) + end + + it "defines termType picklist values" do + vals = described_class::TERM_NOTE_VALUES[:term_type] + expect(vals.values.sort).to eq(%w[ + fullForm acronym abbreviation shortForm variant phrase + ].sort) + end + end + + describe "REF_TYPES" do + it "contains crossReference" do + expect(described_class::REF_TYPES[:cross_reference]) + .to eq("crossReference") + end + end + + describe "XREF_TYPES" do + it "contains externalCrossReference and xGraphic" do + expect(described_class::XREF_TYPES[:external_cross_reference]) + .to eq("externalCrossReference") + expect(described_class::XREF_TYPES[:x_graphic]).to eq("xGraphic") + end + end + + describe "TRANSAC_TYPES" do + it "contains transactionType" do + expect(described_class::TRANSAC_TYPES[:transaction_type]) + .to eq("transactionType") + end + end + + describe "TRANSAC_VALUES" do + it "defines origination and modification" do + vals = described_class::TRANSAC_VALUES[:transaction_type] + expect(vals[:origination]).to eq("origination") + expect(vals[:modification]).to eq("modification") + end + end + + describe "TRANSAC_NOTE_TYPES" do + it "contains responsibility" do + expect(described_class::TRANSAC_NOTE_TYPES[:responsibility]) + .to eq("responsibility") + end + end +end diff --git a/spec/tbx/modules/linguist_spec.rb b/spec/tbx/modules/linguist_spec.rb new file mode 100644 index 0000000..e182e30 --- /dev/null +++ b/spec/tbx/modules/linguist_spec.rb @@ -0,0 +1,45 @@ +# frozen_string_literal: true + +require "spec_helper" + +RSpec.describe Tbx::Modules::Linguist do + describe "ADMIN_TYPES" do + it "contains reading" do + expect(described_class::ADMIN_TYPES[:reading]).to eq("reading") + end + end + + describe "ADMIN_NOTE_TYPES" do + it "contains readingNote" do + expect(described_class::ADMIN_NOTE_TYPES[:reading_note]) + .to eq("readingNote") + end + end + + describe "TERM_NOTE_TYPES" do + it "contains grammaticalNumber, register, transferComment" do + expect(described_class::TERM_NOTE_TYPES[:grammatical_number]) + .to eq("grammaticalNumber") + expect(described_class::TERM_NOTE_TYPES[:register]).to eq("register") + expect(described_class::TERM_NOTE_TYPES[:transfer_comment]) + .to eq("transferComment") + end + end + + describe "TERM_NOTE_VALUES" do + it "defines grammaticalNumber picklist values" do + vals = described_class::TERM_NOTE_VALUES[:grammatical_number] + expect(vals.values.sort).to eq(%w[ + singular plural dual mass otherNumber + ].sort) + end + + it "defines register picklist with 7 values" do + vals = described_class::TERM_NOTE_VALUES[:register] + expect(vals.length).to eq(7) + expect(vals[:colloquial]).to eq("colloquialRegister") + expect(vals[:neutral]).to eq("neutralRegister") + expect(vals[:technical]).to eq("technicalRegister") + end + end +end diff --git a/spec/tbx/modules/min_spec.rb b/spec/tbx/modules/min_spec.rb new file mode 100644 index 0000000..32e0513 --- /dev/null +++ b/spec/tbx/modules/min_spec.rb @@ -0,0 +1,52 @@ +# frozen_string_literal: true + +require "spec_helper" + +RSpec.describe Tbx::Modules::Min do + describe "ADMIN_TYPES" do + it "contains customerSubset" do + expect(described_class::ADMIN_TYPES[:customer_subset]) + .to eq("customerSubset") + end + end + + describe "DESCRIP_TYPES" do + it "contains subjectField" do + expect(described_class::DESCRIP_TYPES[:subject_field]) + .to eq("subjectField") + end + end + + describe "TERM_NOTE_TYPES" do + it "contains administrativeStatus and partOfSpeech" do + expect(described_class::TERM_NOTE_TYPES[:administrative_status]) + .to eq("administrativeStatus") + expect(described_class::TERM_NOTE_TYPES[:part_of_speech]) + .to eq("partOfSpeech") + end + end + + describe "TERM_NOTE_VALUES" do + it "defines administrativeStatus picklist values" do + vals = described_class::TERM_NOTE_VALUES[:administrative_status] + expect(vals.values.sort).to eq(%w[ + admittedTerm-admn-sts deprecatedTerm-admn-sts + preferredTerm-admn-sts supersededTerm-admn-sts + ].sort) + end + + it "defines partOfSpeech picklist values" do + vals = described_class::TERM_NOTE_VALUES[:part_of_speech] + expect(vals.values.sort).to eq(%w[ + adjective adverb noun other verb + ].sort) + end + end + + describe "XREF_TYPES" do + it "contains externalCrossReference" do + expect(described_class::XREF_TYPES[:external_cross_reference]) + .to eq("externalCrossReference") + end + end +end diff --git a/spec/tbx/ref_spec.rb b/spec/tbx/ref_spec.rb new file mode 100644 index 0000000..a2b1354 --- /dev/null +++ b/spec/tbx/ref_spec.rb @@ -0,0 +1,25 @@ +# frozen_string_literal: true + +require "spec_helper" + +RSpec.describe Tbx::Ref do + describe "TYPES" do + it "defines crossReference from Basic" do + expect(described_class::TYPES[:cross_reference]).to eq("crossReference") + end + end + + describe "XML round-trip" do + it "round-trips a ref through XML" do + ref = described_class.new( + type: "crossReference", + target: "c2", + content: ["see also"], + ) + xml = ref.to_xml + parsed = described_class.from_xml(xml) + expect(parsed.type).to eq("crossReference") + expect(parsed.target).to eq("c2") + end + end +end diff --git a/spec/tbx/term_comp_grp_spec.rb b/spec/tbx/term_comp_grp_spec.rb new file mode 100644 index 0000000..88f8e98 --- /dev/null +++ b/spec/tbx/term_comp_grp_spec.rb @@ -0,0 +1,18 @@ +# frozen_string_literal: true + +require "spec_helper" + +RSpec.describe Tbx::TermCompGrp do + describe "XML round-trip" do + it "round-trips a termCompGrp with termComp and note" do + grp = described_class.new( + term_comp: Tbx::TermComp.new(content: ["hydro"]), + note: [Tbx::Note.new(content: ["prefix component"])], + ) + xml = grp.to_xml + parsed = described_class.from_xml(xml) + expect(parsed.term_comp.content.join).to eq("hydro") + expect(parsed.note.length).to eq(1) + end + end +end diff --git a/spec/tbx/term_comp_sec_spec.rb b/spec/tbx/term_comp_sec_spec.rb new file mode 100644 index 0000000..0bd0179 --- /dev/null +++ b/spec/tbx/term_comp_sec_spec.rb @@ -0,0 +1,67 @@ +# frozen_string_literal: true + +require "spec_helper" + +RSpec.describe Tbx::TermCompSec do + describe "TYPES" do + it "defines all 5 TermComp type values" do + expected = %w[ + hyphenation lemma morphologicalElement syllabification termElement + ] + expect(described_class::TYPES.values.sort).to eq(expected.sort) + end + + it "defines hyphenation type" do + expect(described_class::TYPES[:hyphenation]).to eq("hyphenation") + end + + it "defines lemma type" do + expect(described_class::TYPES[:lemma]).to eq("lemma") + end + + it "defines morphologicalElement type" do + expect(described_class::TYPES[:morphological_element]) + .to eq("morphologicalElement") + end + + it "defines syllabification type" do + expect(described_class::TYPES[:syllabification]).to eq("syllabification") + end + + it "defines termElement type" do + expect(described_class::TYPES[:term_element]).to eq("termElement") + end + end + + describe "XML round-trip" do + it "round-trips a termCompSec with type and termComp children" do + sec = described_class.new( + type: "hyphenation", + term_comp: [ + Tbx::TermComp.new(content: ["hydro"]), + Tbx::TermComp.new(content: ["carbon"]), + ], + ) + xml = sec.to_xml + parsed = described_class.from_xml(xml) + expect(parsed.type).to eq("hyphenation") + expect(parsed.term_comp.length).to eq(2) + expect(parsed.term_comp[0].content.join).to eq("hydro") + expect(parsed.term_comp[1].content.join).to eq("carbon") + end + + it "round-trips a termCompSec with termCompGrp children" do + sec = described_class.new( + type: "syllabification", + term_comp_grp: [ + Tbx::TermCompGrp.new(term_comp: Tbx::TermComp.new(content: ["hy"])), + Tbx::TermCompGrp.new(term_comp: Tbx::TermComp.new(content: ["dro"])), + ], + ) + xml = sec.to_xml + parsed = described_class.from_xml(xml) + expect(parsed.type).to eq("syllabification") + expect(parsed.term_comp_grp.length).to eq(2) + end + end +end diff --git a/spec/tbx/term_comp_spec.rb b/spec/tbx/term_comp_spec.rb new file mode 100644 index 0000000..782e78d --- /dev/null +++ b/spec/tbx/term_comp_spec.rb @@ -0,0 +1,21 @@ +# frozen_string_literal: true + +require "spec_helper" + +RSpec.describe Tbx::TermComp do + describe "creation" do + it "creates a term component with text content" do + tc = described_class.new(content: ["hydro"]) + expect(tc.content).to eq(["hydro"]) + end + end + + describe "XML round-trip" do + it "round-trips a termComp through XML" do + tc = described_class.new(content: ["carbon"]) + xml = tc.to_xml + parsed = described_class.from_xml(xml) + expect(parsed.content.join).to eq("carbon") + end + end +end diff --git a/spec/tbx/term_note_spec.rb b/spec/tbx/term_note_spec.rb new file mode 100644 index 0000000..d426878 --- /dev/null +++ b/spec/tbx/term_note_spec.rb @@ -0,0 +1,98 @@ +# frozen_string_literal: true + +require "spec_helper" + +RSpec.describe Tbx::TermNote do + describe "TYPES constants" do + it "defines administrativeStatus type" do + expect(described_class::TYPES[:administrative_status]) + .to eq("administrativeStatus") + end + + it "defines partOfSpeech type" do + expect(described_class::TYPES[:part_of_speech]) + .to eq("partOfSpeech") + end + + it "defines geographicalUsage type" do + expect(described_class::TYPES[:geographical_usage]) + .to eq("geographicalUsage") + end + + it "defines grammaticalGender type" do + expect(described_class::TYPES[:grammatical_gender]) + .to eq("grammaticalGender") + end + + it "defines termLocation type" do + expect(described_class::TYPES[:term_location]) + .to eq("termLocation") + end + + it "defines termType type" do + expect(described_class::TYPES[:term_type]) + .to eq("termType") + end + end + + describe "TYPES completeness" do + it "composes all termNote types from Min, Basic, and Linguist" do + permitted = %w[ + administrativeStatus partOfSpeech + geographicalUsage grammaticalGender termLocation termType + grammaticalNumber register transferComment + ] + expect(described_class::TYPES.values.sort) + .to eq(permitted.sort) + end + end + + describe "standard termNote creation" do + it "creates an administrativeStatus note" do + note = described_class.new( + type: described_class::TYPES[:administrative_status], + content: ["preferredTerm-admn-sts"], + ) + expect(note.type).to eq("administrativeStatus") + expect(note.content).to eq(["preferredTerm-admn-sts"]) + end + + it "creates a partOfSpeech note" do + note = described_class.new( + type: described_class::TYPES[:part_of_speech], + content: ["noun"], + ) + expect(note.type).to eq("partOfSpeech") + expect(note.content).to eq(["noun"]) + end + + it "creates a termType note" do + note = described_class.new( + type: described_class::TYPES[:term_type], + content: ["fullForm"], + ) + expect(note.type).to eq("termType") + end + + it "creates a grammaticalGender note" do + note = described_class.new( + type: described_class::TYPES[:grammatical_gender], + content: ["masculine"], + ) + expect(note.type).to eq("grammaticalGender") + end + end + + describe "XML round-trip" do + it "round-trips a termNote through XML" do + original = described_class.new( + type: "partOfSpeech", + content: ["verb"], + ) + xml = original.to_xml + parsed = described_class.from_xml(xml) + expect(parsed.type).to eq("partOfSpeech") + expect(parsed.content.join).to eq("verb") + end + end +end diff --git a/spec/tbx/transac_note_spec.rb b/spec/tbx/transac_note_spec.rb new file mode 100644 index 0000000..3341c72 --- /dev/null +++ b/spec/tbx/transac_note_spec.rb @@ -0,0 +1,11 @@ +# frozen_string_literal: true + +require "spec_helper" + +RSpec.describe Tbx::TransacNote do + describe "TYPES" do + it "defines responsibility from Basic" do + expect(described_class::TYPES[:responsibility]).to eq("responsibility") + end + end +end diff --git a/spec/tbx/transac_spec.rb b/spec/tbx/transac_spec.rb new file mode 100644 index 0000000..0390b0e --- /dev/null +++ b/spec/tbx/transac_spec.rb @@ -0,0 +1,36 @@ +# frozen_string_literal: true + +require "spec_helper" + +RSpec.describe Tbx::Transac do + describe "TYPES" do + it "defines transactionType from Basic" do + expect(described_class::TYPES[:transaction_type]).to eq("transactionType") + end + end + + describe "VALUES" do + it "defines origination value" do + expect(described_class::VALUES[:transaction_type][:origination]) + .to eq("origination") + end + + it "defines modification value" do + expect(described_class::VALUES[:transaction_type][:modification]) + .to eq("modification") + end + end + + describe "XML round-trip" do + it "round-trips a transac through XML" do + transac = described_class.new( + type: "transactionType", + content: ["origination"], + ) + xml = transac.to_xml + parsed = described_class.from_xml(xml) + expect(parsed.type).to eq("transactionType") + expect(parsed.content.join).to eq("origination") + end + end +end diff --git a/spec/tbx/xref_spec.rb b/spec/tbx/xref_spec.rb new file mode 100644 index 0000000..d8fd88c --- /dev/null +++ b/spec/tbx/xref_spec.rb @@ -0,0 +1,26 @@ +# frozen_string_literal: true + +require "spec_helper" + +RSpec.describe Tbx::Xref do + describe "TYPES" do + it "composes types from Min and Basic modules" do + expected = %w[externalCrossReference xGraphic] + expect(described_class::TYPES.values.sort).to eq(expected.sort) + end + end + + describe "XML round-trip" do + it "round-trips an xref through XML" do + xref = described_class.new( + type: "externalCrossReference", + target: "https://example.com", + content: ["Example"], + ) + xml = xref.to_xml + parsed = described_class.from_xml(xml) + expect(parsed.type).to eq("externalCrossReference") + expect(parsed.target).to eq("https://example.com") + end + end +end