MAGiiCAT V. ORIENTATION of OUTFLOWS and ACCRETION DETERMINE the KINEMATICS and COLUMN DENSITIES of the CIRCUMGALACTIC MEDIUM
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posted on 2024-07-26, 13:56 authored by Nikole NielsenNikole Nielsen, Christopher W. Churchill, Glenn KacprzakGlenn Kacprzak, Michael MurphyMichael Murphy, Jessica L. EvansWe investigate the dependence of gas kinematics and column densities in the MgII-absorbing circumgalactic medium on galaxy color, azimuthal angle, and inclination to trace baryon cycle processes. Our sample of 30 foreground isolated galaxies at 0.3
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DP13010056:ARC
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1538-4357Journal title
Astrophysical JournalVolume
812Issue
1Article number
article no. 83Pagination
11 ppPublisher
IOP PublishingCopyright statement
Copyright © 2015 The American Astronomical Society. The published version is reproduced in accordance with the copyright policy of the publisher and can be also be located at http://doi.org/10.1088/0004-637X/812/1/83.Language
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