Computer Science
Scientific paper
Oct 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop....1h&link_type=abstract
XMM-Newton Proposal ID #04000103
Computer Science
Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Abell 3391, Filament, Abell 3395, Xmm-Newton Proposal 04000103
Scientific paper
We will use the spectro-spatial capability of XMM to map the hot gas of the entire Abell 3395-Abell 3391 region of the Horologium supercluster. In particular, we will: (1) measure the baryon fraction for clusters, groups, and filamentary gas, (2) make temperature, pressure, and entropy maps to search for the merger and infall signatures of the complex Abell 3395 3-body system, (3) construct a dynamical model of the Abell 3395-Abell 3391 filament using the X-ray measured masses combined with the galaxy kinematical parameters obtained from Horologium Consortium collaborators, and (4) work with Horologium Consortium members on a multi-waveband analysis of galaxy evolution in the context of large-scale structure formation.
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