XMM-Newton Proposal 03020302

Details XMM-Newton Proposal 03020302 XMM-Newton Proposal 03020302

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...68f&link_type=abstract

XMM-Newton Proposal ID #03020302

Computer Science

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, A548B, A1664, Xmm-Newton Proposal 03020302

Scientific paper

The clusters A548b and A1664 are peculiar in the radio domain because of the presence of radio relics. These are very extended diffuse radio sources, located in cluster peripheral regions, and associated with the intracluster medium. According to theoretical models, the radio relics are energized by cluster merger shocks. We wish to investigate the cluster X-ray properties, the status of the intracluster medium, the presence of shocks, filaments or cold fronts, in order to analyze the energy transfer between the thermal gas and the radio emitting particles. The study of the connection between X-ray and radio emission will be crucial to understand the formation of relics, and more generally of the non-thermal components in clusters, and their relation to the cluster dynamics.

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