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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/3064
DC FieldValueLanguage
dc.contributor.authorIlić, Draganaen_US
dc.contributor.authorMura, G Laen_US
dc.contributor.authorPopović, Lukaen_US
dc.contributor.authorShapovalova, A Ien_US
dc.contributor.authorCiroi, Sen_US
dc.contributor.authorChavushyan, V Hen_US
dc.contributor.authorRafanelli, Pen_US
dc.contributor.authorBurenkov, A Nen_US
dc.contributor.authorMarcado, Aen_US
dc.date.accessioned2026-01-13T16:37:43Z-
dc.date.available2026-01-13T16:37:43Z-
dc.date.issued2007-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/3064-
dc.description.abstractWe present some results of our study of the physical properties of the broad-line region of active galactic nuclei. We apply the Boltzmann Plot (BP) method to the Balmer lines of 90 AGN from Sloan Digital Sky Survey database, and to the well-studied variable AGN NGC 5548.en_US
dc.language.isoenen_US
dc.publisherAstronomical Society of Pacificen_US
dc.relation.ispartofConference series of Astronomical Society of Pacificen_US
dc.titlePhysical Properties of the Broad-line Regionen_US
dc.typeConference Objecten_US
dc.relation.conferenceWorkshop on Central Engine of Active Galactic Nuclei (2006 ; Xi'An)en_US
dc.relation.publicationThe Central Engine of Active Galactic Nuclei : Proceedings of the Workshop held at Xi'an Jiatong Universityen_US
dc.identifier.isi000251450500106-
dc.contributor.affiliationAstronomyen_US
dc.contributor.affiliationAstronomyen_US
dc.relation.isbn978-1-58381-307-2en_US
dc.description.rankM33en_US
dc.relation.firstpage405en_US
dc.relation.lastpage406en_US
item.openairetypeConference Object-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextnone-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
crisitem.author.deptAstronomy-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-1134-4015-
crisitem.author.orcid0000-0003-2398-7664-
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