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• W2049275573 abstract "In the first part we briefly review the results of the BeppoSAX observations regarding the search for non-thermal emission from clusters of galaxies exploiting the unique spectral capabilities of the PDS. For the first time non-thermal radiation has been detected in the Coma cluster, and then in Abell 2256. In the second part we show a more recent BeppoSAX observation of Abell 754 that reports a non-thermal excess with respect to the thermal emission at energies greater than ∼ 45 keV, at a confidence level slightly above 3σ. The presence of a radio halo in A754, considered the prototype of a merging cluster, reinforces the link between formation of Mpc-scale radio regions and very recent or current merger processes. The radio results combined with the hard X-ray excess detected by BeppoSAX give information on the origin of the electron population responsible for non-thermal phenomena in galaxy clusters." @default.
• W2049275573 created "2016-06-24" @default.
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• W2049275573 date "2004-06-01" @default.
• W2049275573 modified "2023-09-26" @default.
• W2049275573 title "Non thermal emission from Abell 754" @default.
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• W2049275573 doi "https://doi.org/10.1016/j.nuclphysbps.2004.04.005" @default.
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