The Broad Line Region of AGN: Kinematics and Physics

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dc.creatorPopovic, L. C.
dc.date2006-12-23
dc.date.accessioned2026-07-07T10:21:20Z
dc.date.available2026-07-07T10:21:20Z
dc.descriptionIn this paper a discussion of kinematics and physics of the Broad Line Region (BLR) is given. The possible physical conditions in the BLR and problems in determination of the physical parameters (electron temperature and density) are considered. Moreover, one analyses the geometry of the BLR and the probability that (at least) a fraction of the radiation in the Broad Emission Lines (BELs) originates from a relativistic accretion disk.
dc.description11 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0612712
dc.identifierhttp://arxiv.org/abs/astro-ph/0612712
dc.identifierSerb.Astron.J.173:1-11,2006
dc.identifierdoi:10.2298/SAJ0673001P
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175140
dc.subjectAstrophysics
dc.titleThe Broad Line Region of AGN: Kinematics and Physics
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