AGN: The High-Energy Status before INTEGRAL

dc.creatorCollmar, W.
dc.date2001-05-11
dc.date.accessioned2026-07-07T01:58:33Z
dc.date.available2026-07-07T01:58:33Z
dc.descriptionMuch progress in the knowledge of the high-energy emission (>50 keV) from Active Galactic Nuclei has been made during the last decade, predominately by the experiments aboard the Compton Gamma-Ray Observatory. After the end of the CGRO mission and prior to the upcoming INTEGRAL mission the current status of high-energy emission properties and scenarios is summarized for different AGN classes. In addition, prospects for INTEGRAL observations of AGN are given.
dc.description8 pages including 16 figures; invited paper, to appear in the proceedings of the 4th INTEGRAL Workshop 'Exploring the Gamma-Ray Universe', Alicante/Spain, September 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0105193
dc.identifierhttp://arxiv.org/abs/astro-ph/0105193
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2761
dc.subjectAstrophysics
dc.titleAGN: The High-Energy Status before INTEGRAL
dc.typetext

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