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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/3074
DC FieldValueLanguage
dc.contributor.authorBon, Een_US
dc.contributor.authorStanić, Nen_US
dc.contributor.authorIlić, Draganaen_US
dc.contributor.authorKubicela, Aen_US
dc.contributor.authorMediavilla, E Gen_US
dc.contributor.authorPopović, Lukaen_US
dc.date.accessioned2026-01-14T12:27:29Z-
dc.date.available2026-01-14T12:27:29Z-
dc.date.issued2003-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/3074-
dc.description.abstractWe have modelled the central emitting broad line region (BLR) of the III Zw2 using the Hα Hβ Lyα and Mg II (2798) broad lines. We proposed that two-component model, consisting of inner Keplerian relativistic disk and an outer emitting structure that surrounds the disk, can explain the shape of III Zw 2 Broad Linesen_US
dc.language.isoenen_US
dc.publisherBeograd : Astronomska opservatorijaen_US
dc.relation.ispartofPublications of the Astronomical Observatory of Belgrade)en_US
dc.titleTwo-component model for III Zw 2 broad line regionen_US
dc.typeConference Objecten_US
dc.relation.conferenceSerbian Conference on Spectral Line Shapes (4 ; 2003 ; Aranđelovac)en_US
dc.relation.publicationIV Serbian Conference on Spectral Line Shapesen_US
dc.identifier.urlhttps://publications.aob.rs/76/pdf/171-174.pdf-
dc.contributor.affiliationAstronomyen_US
dc.contributor.affiliationAstronomyen_US
dc.relation.issn0373-3742en_US
dc.description.rankM63en_US
dc.relation.firstpage171en_US
dc.relation.lastpage174en_US
dc.relation.issue76en_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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