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 and compare it to identically selected field...
Main Authors: | Rudnick, Gregory, Jablonka, Pascale, Moustakas, John, Aragón-Salamanca, Alfonso, Zaritsky, Dennis, Jaffé, Yara L., Lucia, Gabriella De, Desai, Vandana, Halliday, Claire, Just, Dennis, Milvang-Jensen, Bo, Poggianti, Bianca |
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Other Authors: | Univ Arizona |
Language: | en |
Published: |
IOP PUBLISHING LTD
2017
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Subjects: | |
Online Access: | http://hdl.handle.net/10150/627106 http://arizona.openrepository.com/arizona/handle/10150/627106 |
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