A Critical Test for the Existence of Cooling Gas in the Cores of Galaxy Clusters

Details A Critical Test for the Existence of Cooling Gas in the Cores of Galaxy Clusters A Critical Test for the Existence of Cooling Gas in the Cores of Galaxy Clusters

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop...88m&link_type=abstract

XMM-Newton Proposal ID #04022602

Physics

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Abell 1068, Abell 1068, Xmm-Newton Proposal 04022602

Scientific paper

We propose to obtain a deep, RGS spectrum of the Abell 1068 cluster. The
spectrum will be sensitive enough to measure cooling in the Fe XVII
lines at or below the level of star formation in the cD galaxy. This
measurement is the critical test for the existence of cooling and
feedback processes in the cores of clusters.

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