The Coma Cluster hard X-ray spectrum revisited: still no evidence for a hard tail

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dc.creatorRossetti, M.
dc.creatorMolendi, S.
dc.date2007-02-15
dc.date.accessioned2026-07-07T07:46:59Z
dc.date.available2026-07-07T07:46:59Z
dc.descriptionIn this note, we reply to Fusco-Femiano et al. (2004) and Fusco-Femiano et al. (2006), who cast doubts on our analysis of the PDS observations of the Coma Cluster which we describe in Rossetti & Molendi (2004). We discuss the main issues in Fusco-Femiano et al. (2006) and we confirm that the available data do not allow to firmly establish the presence of a non-thermal component in the hard X-ray spectrum of the Coma cluster.
dc.descriptionelectronic pre-print only, 5 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0702417
dc.identifierhttp://arxiv.org/abs/astro-ph/0702417
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/124010
dc.subjectAstrophysics
dc.titleThe Coma Cluster hard X-ray spectrum revisited: still no evidence for a hard tail
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