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Hard X-Ray Radiation in the Coma Cluster Spectrum

Open access
Fusco-Femiano, Roberto, Dal Fiume, Daniele, Feretti, Luigina, Giovannini, Gabriele, Grandi, Paola, Matt, Giorgio, Molendi, Silvano, Santangelo, Andrea·1999·The Astrophysical Journal

Abstract

Hard X-ray radiation has been detected for the first time in the Coma Cluster by BeppoSAX . Thanks to the unprecedented sensitivity of the Phoswich Detection System (PDS) instrument, the source has been detected up to ~80 keV. There is clear evidence (4.5 σ) for nonthermal emission in excess of thermal emission above ~25 keV. The hard excess is very unlikely to be the result of X Comae, the Seyfert 1 galaxy that is present in the field of view of the PDS. A hard spectral tail that is due to inverse Compton scattering on cosmic microwave background photons is predicted in clusters, like Coma, with radio halos. Combining the present results with radio observations, a volume-averaged intracluster magnetic field of ~0.15 μG is derived, while the electron energy density of the emitting electrons is ~7 × 10 −14 ergs cm -3 .

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Metadata

Authors
Fusco-Femiano, R., Dal Fiume, D., Feretti, L., Giovannini, G., Grandi, P., Matt, G., Molendi, S., & Santangelo, A.
Venue
The Astrophysical Journal
Published
1999-03-01
Volume
513
Issue
1
Pages
L21-L24
ISSN
0004-637X (ISSN-L)
OpenAlex
W1975215917
Cited by
260
References
0
FWCI
22.49
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Hard X-Ray Radiation in the Coma Cluster Spectrum. https://app.cochat.ai/papers/10.1086/311902
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Fusco-Femiano, R., Dal Fiume, D., Feretti, L., Giovannini, G., Grandi, P., Matt, G., Molendi, S., & Santangelo, A. (1999). Hard X-Ray Radiation in the Coma Cluster Spectrum. The Astrophysical Journal. https://doi.org/10.1086/311902

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