Physics
Scientific paper
Oct 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008xmm..prop...99p&link_type=abstract
XMM-Newton Proposal ID #06037510
Physics
Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Rxcj0056.8-5255, Rxcj0056.8-5255, Rxcj1231.0+0037, Rxcj1231.0+0037, Rxcj1122.3+2419, Rxcj1122.3+2419, Rxcj1412.2-3419
Scientific paper
Our current understanding of the X-ray properties of galaxy groups is limited by poor quality data and an inhomogeneous and non-representative coverage of the mass function. We propose to make sufficiently deep observations of a representative X-ray luminosity selected sample of 10 galaxy groups to detect the emission out to ~ R_500 with similar accuracy to that available for observations of nearby clusters. With these data we will investigate the relative importance of gravitational and non-gravitational processes in setting the observed X-ray properties of group scale haloes, via extensive examination of their structural and scaling properties.
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