Study of the most extreme cooling core cluster at z greater 0.3, RXCJ1504.1-0248

Details Study of the most extreme cooling core cluster at z greater 0.3, RXCJ1504.1-0248 Study of the most extreme cooling core cluster at z greater 0.3, RXCJ1504.1-0248

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop...39b&link_type=abstract

XMM-Newton Proposal ID #04010401

Physics

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Rxcj1504.1-0248, Xmm-Newton Proposal 04010401

Scientific paper

In the REFLEX survey we recently discovered the most luminous cluster known in the southern sky at z greater 0.35 (with z=0.21). A CHANDRA observation reveals it as one of the two most dramatic cooling core clusters. Most of the very high X-ray luminosity is actually coming from the cooling core. Both properties make the cluster a prime study object, in particular in the light of the new cooling core physics interpretation with a regulated feedback heating by AGN. In this picture the amount of cooling gas that can be held by the cluster potential against the dispersion by the AGN is actually regulating the amount of mass condensation and AGN Black Hole growth. The proposed observation will shed light on the global structure as well as the thermal structure in the cooling core.

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