XMM-Newton Proposal 03064903

Details XMM-Newton Proposal 03064903 XMM-Newton Proposal 03064903

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..210s&link_type=abstract

XMM-Newton Proposal ID #03064903

Computer Science

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Abell 2204, Abell 2204, Abell 2204, Xmm-Newton Proposal 03064903

Scientific paper

We propose to make a 60 ks observation using XMM-Newton of the luminous galaxy cluster Abell 2204. Using this observation we wish to study the 100 kpc (1 arcmin) radius high abundance ring we found using Chandra. XMM will allow us to resolve this ring into many different spatial components, and measure the abundances to high accuracy. In addition, the cluster displays a large range of temperature (3-12 keV), and is an idea target to search for the existence of cool X-ray emitting gas. The central galaxy in this cluster is rich in cold gas. We will provide upper limits of 130 Msun/yr (3-sigma) for gas around 0.3 keV. We will be sensitive to any cooling of gas to below 0.1 keV at a rate exceeding 100 Msun/yr.

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