XMM-Newton Proposal 02044601

Details XMM-Newton Proposal 02044601 XMM-Newton Proposal 02044601

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..237f&link_type=abstract

XMM-Newton Proposal ID #02044601

Computer Science

Klemola 44, Xmm-Newton Proposal 02044601

Scientific paper

We propose to observe a nearby galaxy cluster Klemola 44 with a 20 ksec exposure. One of the recent interesting results found in many cD clusters by Chandra and XMM is a relation between radio and X-ray emission in the cluster core region. Klemola 44 has a radio relic near the cD galaxy, which is a good oppotunity to look into the relation in an early stage of relic evolution. A lower luminosity of central cool components than expected by cooling flow model is now the most interest and problematic topic in cD clusters. The central temperature map and cool emission from galaxies, which are now merging together into a big cD galaxy in this cluster, will give us rich information of the cooling flow problem in comparison with the results of cD clusters.

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