The Abell 1882 Supergroup: Star-formation And Agn Activity At The Moment Of Collapse

Details The Abell 1882 Supergroup: Star-formation And Agn Activity At The Moment Of Collapse The Abell 1882 Supergroup: Star-formation And Agn Activity At The Moment Of Collapse

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21641801m&link_type=abstract

American Astronomical Society, AAS Meeting #216, #418.01; Bulletin of the American Astronomical Society, Vol. 41, p.829

Astronomy and Astrophysics

Astronomy

Scientific paper

Abell 1882 is a clump of three or four galaxy groups that will likely collapse into a galaxy cluster. Unlike super-clusters, this ``super-group'' is an excellent laboratory to study how galaxies are pre-processed by the group environment before they settle into their tranquil lives inside galaxy clusters. We utilize ground-based imaging and spectroscopy, as well as X-ray data for the intracluster medium to map out the local galaxy, gas, and dark matter densities. We examine how the star-formation and AGN properties of the bright galaxies are distributed. Our aim is to understand what physical mechanisms in Abell 1882 are responsible for the transformation of field-galaxies into cluster galaxies.

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