Scaling Relations for Low-Mass Galaxy Clusters and Groups

Details Scaling Relations for Low-Mass Galaxy Clusters and Groups Scaling Relations for Low-Mass Galaxy Clusters and Groups

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cxo..prop.2446v&link_type=abstract

Chandra Proposal ID #09800349

Statistics

Chandra Proposal Id #09800349

Scientific paper

Detailed measurements of the cluster scaling relations (e.g., L-T) require 1) large, objectively selected, statistically complete samples, and 2) observations that cover a large fraction of the system's virial radius. Such data are now available in the Chandra archive for a large number of high-M clusters, but not for the systems with T ~ 2 keV and below. We propose to fill this gap by observing a sample of 22 low-L objects from a new, sensitive X-ray survey. These observations will quadruple the statistics for low-T clusters and extend the reliable determination

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