Large Scale ICM Properties of PerseusII - Correcting for Anisotropies

Details Large Scale ICM Properties of PerseusII - Correcting for Anisotropies Large Scale ICM Properties of PerseusII - Correcting for Anisotropies

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..202d&link_type=abstract

XMM-Newton Proposal ID #04054102

Other

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Perseus Offset, Perseus Offset, Xmm-Newton Proposal 04054102

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 templates to test the biases introduced by simplifications used in the analysis of more distant clusters. Perseus stands out as the optimal choice for such analysis, due to its brightness, proximity, and ubiquitous physical properties. We propose 2 short pointings that, together with other archived ones, will allow us to fully 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 presence and extent of ICM velocity gradient.

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