Astronomy and Astrophysics – Astronomy
Scientific paper
May 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21811906f&link_type=abstract
American Astronomical Society, AAS Meeting #218, #119.06; Bulletin of the American Astronomical Society, Vol. 43, 2011
Astronomy and Astrophysics
Astronomy
Scientific paper
Galaxy groups are increasingly recognized as a key environment for transforming galaxy morphologies and star formation rates. Current research is focused on illuminating specific physical processes responsible for galaxy evolution in these systems. Super-Group 1120-12 consists of four virialized groups at z 0.36 that will merge and form a cluster comparable in mass to Coma by the current epoch. Using multiwavelength (X-ray, UV, Optical, 24 micron, Radio) imaging and spectroscopic data we identify numerous AGN, starburst, and star-forming galaxies and characterize their associated outflows and physical properties in the context of the group environment.
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