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arXiv:1205:0245Galaxy Orientation90°M104BlueRed0°OutflowsMore MgIIInflowsLess MgIIM82

Lightcurve Analysis and Photometry on CCD Images of Asteroids ...

Circle Packing Approach to Modeling van der Waals Forces

arXiv:1205:0245Galaxy Orientation90°M104BlueRed0°OutflowsMore MgIIInflowsLess MgIIM82

Conclusions• Studying the CGM is crucial to understandinggalaxy evolution• MAGIICAT – Largest sample of MgII galaxies• The properties of the CGM strongly depend onthe host galaxy color, luminosity, and halomass• Bluer, brighter, and more massive galaxies have moregas out to further distances, and have less patchygaseous halos.• Galaxy orientation mattersThank you!

Page 2 and 3: The Circumgalactic Medium• Reserv
Page 4 and 5: Nielsen et al. 2013, in prepMAGIICA
Page 6 and 7: arXiv:1211.1008, arXiv:1211.1380Amo
Page 8 and 9: arXiv:1211.1008, arXiv:1211.1380Cov

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