From 96388e9207fe087c8b104fdb77c04fa2b061f363 Mon Sep 17 00:00:00 2001 From: Alexander Ji Date: Mon, 15 Jun 2015 14:36:04 -0400 Subject: [PATCH] Removed plots from satelliteplanes; will redo this page after paper is submitted --- science/satelliteplanes/index.md | 29 +---------------------------- 1 file changed, 1 insertion(+), 28 deletions(-) diff --git a/science/satelliteplanes/index.md b/science/satelliteplanes/index.md index fbdef66..d05d207 100644 --- a/science/satelliteplanes/index.md +++ b/science/satelliteplanes/index.md @@ -7,31 +7,4 @@ Project Lead: Alex Ji (alexji@mit.edu) Here is the poster presented at University of Michigan Local Group Astrostatistics Conference: PDF -A paper is in preparation, expected submission in late June. In the meantime, here are some additional plots that were of interest to people at the conference. - -## Radial Profiles -Satellite position radial profiles compared to the 11 classical Milky Way satellites. -The colored lines correspond to different choices of satellites. Blue lines are the first 11 satellites by Vpeak, Green lines are satellites with stellar mass > 10^5.5 Msun, Red lines are satellites with stellar mass > 10^5 Msun. Stellar masses found by Moster et al. 2013 abundance matching. - -
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- -## Orbital alignment with plane -Here we plot the cumulative number of satellites whose angular momentum is within a certain angle of the plane's minor axis. Solid lines indicate total number pointing in either direction (i.e. co-rotating and anti-co-rotating). Dashed lines indicate total number pointing in single direction. - -
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- -## Edge-On and Face-On Satellite Distributions -Here are the spatial positions of the satellites relative to the best-fit plane. The colored dots are satellites with stellar mass > 10^5 Msun (the red lines in previous plots). Arrows indicate where the satellite will travel in 1Myr given its current velocity. - -
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- +A paper is in preparation, expected submission in late June.