Determining the halo mass scale where galaxies lose their gas

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Determining the halo mass scale where galaxies lose their gas

A major question in galaxy formation is how the gas supply that fuels activity in galaxies is modulated by their environment. We use spectroscopy of a set of well characterized clusters and groups at $0.4<z<0.8$ from the ESO Distant Cluster Survey (EDisCS) and compare it to identically selecte...

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Bibliographic Details
Main Authors:	Rudnick, Gregory, Jablonka, Pascale, Moustakas, John, Aragón-Salamanca, Alfonso, Zaritsky, Dennis, Jaffe, Yara L., De Lucia, Gabriella, Desai, Vandana, Halliday, Claire, Just, Dennis, Milvang-Jensen, Bo, Poggianti, Bianca
Format:	Article
Published:	American Astronomical Society 2017
Subjects:	Astrophysics - Astrophysics of Galaxies
Online Access:	https://eprints.nottingham.ac.uk/47311/

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