Other
Scientific paper
Jan 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21533001c&link_type=abstract
American Astronomical Society, AAS Meeting #215, #330.01; Bulletin of the American Astronomical Society, Vol. 42, p.427
Other
Scientific paper
Galaxy groups are evolving environments which display diverse properties even at fixed redshift. The majority of galaxies in the Universe lie in these groups which range from 'poor' systems containing few galaxies (commonly identified via optical selection methods) to massive groups (often identified via X-ray emission from the Intra-Group Medium, IGM). Local studies reveal the galaxy populations of groups vary from being dominated by early (as in typical clusters) to late-type (as in the field population) galaxies. Thus groups are interesting in their own right and also as an environment which affects the evolution of their member galaxies. In order to study groups spanning a significant mass and evolutionary range, we have defined two samples, one via optical spectroscopy and the other via X-ray emission. Both samples contain 25 groups and span a redshift range of 0.04
Balogh Michael L.
Bower Richard G.
Connelly Jennifer L.
Finoguenov Alexis
McGee Sean L.
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