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 (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/

Internet

https://eprints.nottingham.ac.uk/47311/

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