High-energy X emission from the coma cluster

Details High-energy X emission from the coma cluster High-energy X emission from the coma cluster

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...397..438r&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 397, no. 2, p. 438-441.

Astronomy and Astrophysics

Astrophysics

4

Emission Spectra, Galactic Clusters, X Ray Sources, Diffuse Radiation, Interstellar Gas, Radio Emission

Scientific paper

A detailed assessment is given of conflicting high-energy X measurements of the Coma cluster region. Various considerations lead to the conclusion that the recent detection of intense emission in the band 18-130 keV is very unlikely to be diffuse intracluster emission from the Coma cluster. Therefore, the detection of diffuse intracluster emission would require detector sensitivity better than a few 10 exp -6/sq cm/s/keV in the few tens of keV range. If the observed emission originates in the Seyfert galaxy X Comae, its implied X luminosity would make it one of the strongest currently known high-energy X sources.

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