AGN Feedback and Star Formation in the Cooling Flow Cluster RBS797

Details AGN Feedback and Star Formation in the Cooling Flow Cluster RBS797 AGN Feedback and Star Formation in the Cooling Flow Cluster RBS797

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..112g&link_type=abstract

XMM-Newton Proposal ID #05029401

Computer Science

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Rbs 797, Xmm-Newton Proposal 05029401

Scientific paper

We propose to observe the X-ray cavity cluster RBS797, in which radio emission is seen on three different scales and orientations and a massive starburst is found at its center. With the requested observation we aim to: 1) determine the global properties of the cluster (temperature, mass, luminosity) and assess its conformity to scaling relations in order to investigate the potential impact of AGN feedback; 2) compare cooling rate or limits with the star formation rate; 3) investigate the nature of the large-scale radio emission by using the X-ray properties as input to test the electron reacceleration model for the origin of radio mini-halos; 4) study the ICM enrichment process by means of a metallicity map.

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