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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/95
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dc.contributor.authorIlić, Draganaen_US
dc.contributor.authorLa Mura, G.en_US
dc.contributor.authorPopovi, L. Ĉen_US
dc.contributor.authorShapovalova, A. I.en_US
dc.contributor.authorCiroi, S.en_US
dc.contributor.authorChavushyan, V. H.en_US
dc.contributor.authorRafanelli, P.en_US
dc.contributor.authorBurenkov, A. N.en_US
dc.contributor.authorMarcado, A.en_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/123456789/95-
dc.description.abstractWe apply the Boltzmann-Plot (BP) method to the Balmer lines to estimate the physical propertiesin the Broad Line Region of Active Galactic Nuclei. We study the Balmer lines of a sample of 90 AGN from Sloan Digital Sky Survey database, as well as the time variability of the BP parameter A of NGC 5548. © 2007 International Astronomical Union.en
dc.relation.ispartofProceedings of the International Astronomical Unionen_US
dc.subject(galaxies:) quasars: emission linesen
dc.subjectGalaxies: activeen
dc.subjectGalaxies: Seyferten
dc.titlePhysical properties of emitting plasma near massive black holes: The Broad Line Regionen_US
dc.typeConference Paperen_US
dc.relation.publicationBlack Holes from Stars to Galaxies – Across the Range of Massesen_US
dc.identifier.doi10.1017/S174392130700556X-
dc.identifier.scopus2-s2.0-37049015826-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/37049015826-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage383en_US
dc.relation.lastpage384en_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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