Probing structure formation physics with the evolution of cluster properties

Details Probing structure formation physics with the evolution of cluster properties Probing structure formation physics with the evolution of cluster properties

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..106a&link_type=abstract

XMM-Newton Proposal ID #04027502

Physics

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Rxj0221.1+1958, Rxj0030.5+2618, Xmm-Newton Proposal 04027502

Scientific paper

We have been awarded a Large Program in AO4 to study the evolution of cluster structural and scaling properties, using a large sample of distant clusters (z~ 0.5) covering a wide dynamic range in mass (2.5 < kT < 12 keV). Our aim is to provide new insight into the physics of structure formation, both for the dark matter and the baryonic components. We propose to re-observe 2 targets, the observations of which are dramatically affected by flares. To complete the kT > 5 keV range coverage of our sample, we also propose to observe 3 clusters, for which no time was allocated in AO4.

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