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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/123
DC FieldValueLanguage
dc.contributor.authorIlić, Draganaen_US
dc.date.accessioned2022-08-06T16:07:55Z-
dc.date.available2022-08-06T16:07:55Z-
dc.date.issued2009-01-01-
dc.identifier.issn00046280-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/123-
dc.description.abstractThe diagnostics of the physical properties of the broad line region (BLR) of active galactic nuclei (AGN) is still an interesting question. Here we present an overview of our recent investigations of the physics of the BLR using the broad emission lines. © 2009. The Astronomical Society of the Pacific. All rights reserved.en_US
dc.relation.ispartofPublications of the Astronomical Society of the Pacificen_US
dc.titlePlasma diagnostics in the broad line region of active galactic nuclei using emission linesen_US
dc.typeArticleen_US
dc.identifier.doi10.1086/649506-
dc.identifier.scopus2-s2.0-73549086994-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/73549086994-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage1440en_US
dc.relation.lastpage1441en_US
dc.relation.volume121en_US
dc.relation.issue886en_US
item.fulltextNo Fulltext-
item.openairetypeArticle-
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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