A hard X ray observation of the Coma Cluster

Details A hard X ray observation of the Coma Cluster A hard X ray observation of the Coma Cluster

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..901b&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 2: AGN and the X Ray Background p 901-903 (SEE N90-258

Astronomy and Astrophysics

Astronomy

Cluster Analysis, Image Analysis, Star Clusters, X Ray Astronomy, X Ray Spectra, Background Radiation, Data Processing, Data Reduction, Proportional Counters, Scintillation Counters, Statistical Analysis

Scientific paper

Preliminary results of a hard X-ray measurement of the Coma Cluster of galaxies are presented. They were obtained with the MIFRASO (Milan-Frascati-Southampton) telescope on 15 Jul. 1987. High energy component was detected between 30 and 130 keV at a level of 4.4 standard deviation with scintillation detectors covering the energy range 20 to 300 keV. The analysis of the data obtained with the proportional counters on board the same experiment is presented.

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