Determining the Halo Mass Scale Where Galaxies Lose Their Gas

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...

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Bibliographic Details
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
Other Authors: Univ Arizona
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
galaxies: evolution
galaxies: groups: general
galaxies: ISM
Online Access:http://hdl.handle.net/10150/627106
http://arizona.openrepository.com/arizona/handle/10150/627106

Internet

http://hdl.handle.net/10150/627106
http://arizona.openrepository.com/arizona/handle/10150/627106

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