Cluster and galaxy interactions in dense environment: Shapley supercluster core

Details Cluster and galaxy interactions in dense environment: Shapley supercluster core Cluster and galaxy interactions in dense environment: Shapley supercluster core

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009xmm..prop...53b&link_type=abstract

XMM-Newton Proposal ID #06515902

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Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Sc1329-313, Sc1329-312

Scientific paper

The Shapley Supercluster core hosts a remarkably dense structure showing three galaxy clusters --A3562 A3558, A3556-- and two galaxy groups --SC1327-312, SC1329-313-- connected to each other by a filament of hot gas and galaxies. A combined analysis of X-ray and optical data will enable us to investigate thermodynamics of the ICM overcoming group and cluster interactions, and constrain the influence of galaxy-ICM interactions in the global budget of the environmental effects affecting galaxy evolution. We will further search for X-ray emission from the hottest phase of the WHIM, by separating ICM and filament emissions. Following an AO8 proposal, this proposal aims at re-observing a region where pointings are contaminated by soft protons and extending the observed area.

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