The X-ray coolest gas in nearby cool core clusters

Details The X-ray coolest gas in nearby cool core clusters The X-ray coolest gas in nearby cool core clusters

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..176f&link_type=abstract

XMM-Newton Proposal ID #05047806

Physics

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Abell 262, Abell 262, Abell 3581, Abell 3581, Hcg 62, Hcg 62, Xmm-Newton Proposal 05047806

Scientific paper

We propose to make deep RGS observations of three low redshift clusters in order to make definitive statements about the range of temperature in the clusters and the level and spatial distribution of cooling. All three clusters have cool cores, short central cooling times and central radio sources making bubbles. The targets all show FeXVII emission lines, and as they are nearby we are able to spatially resolve the innermost region where the feedback must originate. These observations will exploit the unique capability of the RGS, and build on one of XMM s major discoveries.

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