The Abell 3395-Abell 3391 Filament in the Horologium Supercluster
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We will use the spectrospatial capability of XMM to map the hot gas of theentire Abell 3395Abell 3391 region of the Horologium supercluster. Inparticular, we will: (1) measure the baryon fraction for clusters, groups, andfilamentary gas, (2) make temperature, pressure, and entropy maps to search forthe merger and infall signatures of the complex Abell 3395 3body system, (3)construct a dynamical model of the Abell 3395Abell 3391 filament using theXray measured masses combined with the galaxy kinematical parameters obtainedfrom Horologium Consortium collaborators, and (4) work with HorologiumConsortium members on a multiwaveband analysis of galaxy evolution in thecontext of largescale structure formation. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]



