The high energy emission from black holes

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dc.creatorCaballero-Garcia, M. D.
dc.creatorMiller, J. M.
dc.creatorKuulkers, E.
dc.date2007-11-06
dc.date.accessioned2026-07-07T08:40:58Z
dc.date.available2026-07-07T08:40:58Z
dc.descriptionThe origin of the high energy emission (X-rays and gamma-rays) from black holes is still a matter of debate. We present new evidence that hard X-ray emission in the low/hard state may not be dominated by thermal Comptonization. We present an alternative scenario for the origin of the high energy emission that is well suited to explain the high energy emission from GRO J1655-40.
dc.descriptionSubmitted proceedings to the workshop "X-rays from Nearby Galaxies" (ESAC, Madrid, 5-7 September 2007). Appearing as an MPE report
dc.identifierhttps://arxiv.org/abs/0711.0844
dc.identifierhttp://arxiv.org/abs/0711.0844
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/141536
dc.subjectAstrophysics
dc.titleThe high energy emission from black holes
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