AGN-ICM interaction and peculiar radio emission in the cool core cluster RBS 797

Details AGN-ICM interaction and peculiar radio emission in the cool core cluster RBS 797 AGN-ICM interaction and peculiar radio emission in the cool core cluster RBS 797

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop...58g&link_type=abstract

XMM-Newton Proposal ID #06714001

Computer Science

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Rbs 797

Scientific paper

We propose to observe the X-ray cavity cluster RBS797, which has a massive central starburst and a unique radio source that exhibits large changes in orientation with scale. With the requested observation we aim at: 1) determining the global properties of the cluster (temperature, metallicity, mass, gas mass fraction) up to ~1.3 Mpc (~0.5 r_vir), and investigating the potential impact of AGN feedback on scaling relations; 2) characterizing the AGN/ICM interaction by investigating the nature of the extended radio emission; 3) comparing the cooling rate or limits with the star formation rate.

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