XMM survey of the Fornax cluster up to 0.3 of the virial radius

Details XMM survey of the Fornax cluster up to 0.3 of the virial radius XMM survey of the Fornax cluster up to 0.3 of the virial radius

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop...27m&link_type=abstract

XMM-Newton Proposal ID #05509315

Physics

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Fornax Offset A, Fornax Offset B, Fornax Offset C, Fornax Offset D, Fornax Offset E, Fornax Offset F, Fornax Offset G, Fornax Offset H, Fornax Offset I, Fornax Offset J, Fornax Offset K, Fornax Offset L, Fornax Offset M, Fornax Offset N, Fornax Offset O, Xmm-Newton Proposal Id #05509315

Scientific paper

Groups of galaxies and poor clusters of galaxies are best laboratories for studying history of the universe. The Fornax cluster is the nearest (about 20 Mpc) poor cluster with the smallest-iron mass-to-light ratio. In order to study temperature, entropy and metal distribution and constrain metal enrichment and thermal history in the intracluster medium, we propose to survey the Fornax cluster up to 0.3 times of the virial radius.

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