Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/2880
DC FieldValueLanguage
dc.contributor.authorIlić, Draganaen_US
dc.contributor.authorPopović, Lukaen_US
dc.contributor.authorŠapovalova, Allaen_US
dc.contributor.authorLeón-Tavares, Jen_US
dc.contributor.authorChavushyan, V Hen_US
dc.date.accessioned2025-11-05T09:01:52Z-
dc.date.available2025-11-05T09:01:52Z-
dc.date.issued2010-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/2880-
dc.description.abstractThe structure of the broad line region (BLR) of active galactic nuclei (AGN) can be very complex. Different models have been proposed to explain the kinematics of the BLR (e.g. disk, spherical region, bi-conical outflows, etc.), but so far there is no unique model which would explain all the observed properties of the broad emission line (BEL) profiles. Here we discuss the possibility that an accelerating outflow can affect BEL profiles. We found that in some AGN (as e.g. NGC 4151) the outflow model can well describe the BEL profiles in different epochsen_US
dc.language.isoenen_US
dc.publisherAstronomical society of the Pacificen_US
dc.relation.ispartofAstronomical society of the Pacific Conference Seriesen_US
dc.titlePossible Outflow in the Broad Line Region of Active Galactic Nucleien_US
dc.typeConference Objecten_US
dc.relation.conferenceAccretion and Ejection in AGN: a Global View (2009 ; Como)en_US
dc.relation.publicationAccretion and Ejection in AGN: a Global Viewen_US
dc.identifier.isi000289881400021-
dc.identifier.urlhttp://aspbooks.org/a/volumes/table_of_contents/?book_id=477-
dc.relation.isbn978-1-58381-734-6en_US
dc.description.rankM33en_US
dc.relation.firstpage110en_US
dc.relation.lastpage111en_US
dc.relation.volume427en_US
item.openairetypeConference Object-
item.fulltextNo Fulltext-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-1134-4015-
Appears in Collections:Research outputs
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