Accretion to the Cluster of Galaxies and X-Ray Emission

Details Accretion to the Cluster of Galaxies and X-Ray Emission Accretion to the Cluster of Galaxies and X-Ray Emission

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pthph..53..646t&link_type=abstract

Progress of Theoretical Physics, Vol. 53, No. 3, pp. 646-655

Physics

6

Scientific paper

The X-ray emission from a cluster of galaxies, in particular, from Coma cluster is investigated for the case of steady and spherically symmetric accretion of hot intercluster plasma. The luminosity, the emission region and the X-ray spectrum in 0.1-20 keV region are well explained by this model. It is also shown that the diffuse background X-ray below 20 keV is explained by superpositions of all clusters and of hot intercluster plasma. Also, the thermal structure and history of the universe are discussed.

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