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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/97
DC FieldValueLanguage
dc.contributor.authorBon, E.en_US
dc.contributor.authorPopović, L. Čen_US
dc.contributor.authorIlić, Draganaen_US
dc.date.accessioned2022-08-06T15:18:34Z-
dc.date.available2022-08-06T15:18:34Z-
dc.date.issued2006-08-01-
dc.identifier.issn17439213en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/97-
dc.description.abstractWe modeled the single-peaked Broad Emission Lines (BELs) with two-component model (accretion disk, with surrounding spherical region), comparing it with observational line profiles for a number of Active Galactic Nuclei (AGN). We find that the accretion in the Broad Line Region (BLR) can be present even if the profiles of BELs are single-peaked. © 2007 International Astronomical Union.en
dc.relation.ispartofProceedings of the International Astronomical Unionen_US
dc.subjectAccretion, accretion disksen
dc.subjectGalaxies: nucleien
dc.subjectGalaxies: Seyferten
dc.subjectQuasars: emission linesen
dc.titleAccretion in the broad line region of active galactic nucleien_US
dc.typeConference Paperen_US
dc.relation.publicationBlack Holes from Stars to Galaxies – Across the Range of Massesen_US
dc.identifier.doi10.1017/S1743921307005297-
dc.identifier.scopus2-s2.0-37049020412-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/37049020412-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage329en_US
dc.relation.lastpage330en_US
dc.relation.volume2en_US
dc.relation.issueS238en_US
item.fulltextNo Fulltext-
item.openairetypeConference Paper-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-1134-4015-
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