XMM-Newton Proposal 03057203

Details XMM-Newton Proposal 03057203 XMM-Newton Proposal 03057203

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..184d&link_type=abstract

XMM-Newton Proposal ID #03057203

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Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Perseus Offset1, Perseus Offset3, Xmm-Newton Proposal 03057203

Scientific paper

Nearby galaxy clusters present a unique opportunity to study the spatial variation of the physical properties of the ICM and they also provide us with templates to test the biases introduced by simplifications assumed in the analysis of more distant clusters. Perseus stands out as the optimal choice for such an analysis, due to its brightenss, proximity, and ubiquitous physical characteristics. We propose 4 short observations that will allow us to completely map SN Type enrichment, gas bulk velocities, and other physical parameters up to ~0.3-0.4 of its virial radius. This analysis will address several current issues, such as the excess SN Ia pollution in the outer cluster regions and the claimed presence of velocity gradients in the ICM.

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