AGN Feedback and Cluster Environment

Details AGN Feedback and Cluster Environment AGN Feedback and Cluster Environment

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011scgg.conf....8d&link_type=abstract

"Structure in Clusters and Groups of Galaxies in the Chandra Era, 2011 Chandra Science Workshop held July 12-14, 2011. Edited by

Computer Science

Scientific paper

I will review the evidence for a link between the intracluster gas in the core of the host cluster or group and the activity exhibited by the AGN in the central bright galaxy. The presence of luminous radio activity appears to require low-entropy, X-ray emitting gas, either in the form of a cluster-scale cool core or a more compact, galaxy-scale corona. The large fraction of X-ray luminous clusters whose brightest cluster galaxies are also radio galaxies (and emission-line systems) implies that the relationship is common and relatively long-lived.

Affiliated with

Also associated with

No associations

Rating

AGN Feedback and Cluster Environment 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 AGN Feedback and Cluster Environment, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and AGN Feedback and Cluster Environment will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1667402