Multiwavelength Observations of an Assembling Galaxy Cluster : AGN Content

Details Multiwavelength Observations of an Assembling Galaxy Cluster : AGN Content Multiwavelength Observations of an Assembling Galaxy Cluster : AGN Content

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21924614f&link_type=abstract

American Astronomical Society, AAS Meeting #219, #246.14

Astronomy and Astrophysics

Astronomy

Scientific paper

Galaxy groups are increasingly recognized as a key environment for transforming galaxy morphologies and star formation rates. Super-Group 1120-12 consists of four virialized groups at z 0.37 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, star-forming, and composite galaxies and compare their frequency to that found in cluster and field environments.

Affiliated with

Also associated with

No associations

Rating

Multiwavelength Observations of an Assembling Galaxy Cluster : AGN Content does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Multiwavelength Observations of an Assembling Galaxy Cluster : AGN Content, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multiwavelength Observations of an Assembling Galaxy Cluster : AGN Content will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1579383