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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/99
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dc.contributor.authorIlić, Draganaen_US
dc.contributor.authorPopović, L. Čen_US
dc.contributor.authorCiroi, S.en_US
dc.contributor.authorRafanelli, P.en_US
dc.date.accessioned2022-08-06T15:18:34Z-
dc.date.available2022-08-06T15:18:34Z-
dc.date.issued2008-12-01-
dc.identifier.issn14052059en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/99-
dc.description.abstractDiagnostics of the physical properties in the Broad Line Region (BLR) of Active Galactic Nuclei (AGN) is a difficult subject to study since there is no simple and direct method as is a case for the Narrow Line Region. We propose here a direct method for the temperature estimates in the BLR, that is using the broad Balmer and helium lines (He II A4686 and He I λ5876). © 2008: Instituto de Ashonomía.en
dc.relation.ispartofRevista Mexicana de Astronomia y Astrofisica: Serie de Conferenciasen
dc.titleTemperature diagnostics of the broad line region in Active Galactic Nucleiien_US
dc.typeConference Paperen_US
dc.identifier.scopus2-s2.0-67650449920-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/67650449920-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage102en
dc.relation.volume32en
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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