Hard X-Ray Excesses in Clusters of Galaxies and Their Non-Thermal Origin
2004
The first part of the paper reports all the results obtained by BeppoSAX observations concerning the search for non-thermal components in the spectra of clusters of galaxies, while the origin of the hard X-ray excesses detected in Coma, A2256 and, at lower confidence level, in A754 is discussed in the second part.
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