Detailed Diagnostics of the Nuclear Explosion in the Hydra A Galaxy Cluster

Details Detailed Diagnostics of the Nuclear Explosion in the Hydra A Galaxy Cluster Detailed Diagnostics of the Nuclear Explosion in the Hydra A Galaxy Cluster

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..161b&link_type=abstract

XMM-Newton Proposal ID #05042601

Physics

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Hydra A (I), Xmm-Newton Proposal 05042601

Scientific paper

We propose to use the superior spectro-imaging capabilities of XMM-Newton to shed further light on the heating process in cluster cooling cores by a deep study of the radio lobe-ICM interaction and shock heating in the Hydra A cluster. Encouraged by our findings in the less energetic nearby system M87, we plan to apply the developed diagnostic tools to Hydra A, which shows a wealth of interaction features and resembles as a scaled-up version of M87 seen at a correspondingly larger distance. In particular we want to study the large-scale shock, the entropy structure of the interaction region of the ICM with the outer radio lobes and use the metallicity distribution for further diagnostics.

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