XMM-Newton Proposal 02047202

Details XMM-Newton Proposal 02047202 XMM-Newton Proposal 02047202

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..251f&link_type=abstract

XMM-Newton Proposal ID #02047202

Physics

A426 East1, A426 East2, Xmm-Newton Proposal 02047202

Scientific paper

X-ray mapping of the Perseus cluster, the brightest cluster in the X-ray sky, with XMM-Newton is the most effective way to study physics of cluster dynamics. In the east region of this cluster, ASCA showed remarkable temperature features including an enormous cool region bounded by a hot ridge in the east, which is most possibly caused by a subcluster merger. We propose 7 pointings (including 2 pointings of AO2/Pri-C) for a total of 140 ksec to cover most of the unobserved regions in the Perseus cluster, which will give us a detailed view about the gas heating process and metal distribution.

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