Physics
Scientific paper
Oct 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..140m&link_type=abstract
XMM-Newton Proposal ID #03039501
Physics
Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Ms0735.7+7421, Xmm-Newton Proposal 03039501
Scientific paper
We propose to obtain a deep image of the redshift z=0.22 cluster MS0735.6+7421. The cluster's enormous system of cavities and shocks are depositing 5-8E61erg into the ICM. Heating the cluster at a level of ~1/2 keV per particle, this is enough energy to quench a 200 M0/yr cooling flow for several Gyr and to ``preheat'' the cluster. The image will be used to examine the impact of AGN heating on the L-T relation, to constrain the temperature of the gas filling the cavities, to measure the temperature jump across the shock, and to search for evidence of earlier outbursts.
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