Probing the Gas Content of Galaxy Groups: A Radio Perspective

Details Probing the Gas Content of Galaxy Groups: A Radio Perspective Probing the Gas Content of Galaxy Groups: A Radio Perspective

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...20913901w&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #139.01; Bulletin of the American Astronomical Society,

Astronomy and Astrophysics

Astronomy

Scientific paper

The current state of our understanding of the nature of the gas content of galaxy groups, derived largely from a large body of X-ray observations, leaves us with two key questions. First, what are the relative fractions of the hot, warm/hot, and neutral gas in galaxy groups, and how is each phase distributed within groups? Second, how has the gas content of galaxy groups evolved over time and what is its relationship to the dynamical evolution of the group? The results from a number of investigations of the HI content and deep searches for diffuse synchrotron emission in groups are now shedding light on the evolution of the gas content of galaxy groups.

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