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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/2994
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dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorShapovalova, A Ien_US
dc.contributor.authorPopović, Luka Čen_US
dc.contributor.authorBurenkov, A Nen_US
dc.contributor.authorChavushyan, Ven_US
dc.date.accessioned2025-12-12T15:52:18Z-
dc.date.available2025-12-12T15:52:18Z-
dc.date.issued2009-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/2994-
dc.description.abstractUsing a set of observations of NGC 4151 from 1996 to 2006, we apply 1D and 2D reverberation mapping in order to find dimension of the BLR as well as its kinematical structure. We found that that the BLR size is very compact, as well as different response of the line core and wings to the continuum variation.en_US
dc.language.isoenen_US
dc.publisherBeograd : Astronomska opservatorijaen_US
dc.relation.ispartofPublications de l'Observatoire Astronomique de Beograden_US
dc.title1D and 2D Reverberation Mapping Applied on H_beta Line of NGC 4151en_US
dc.typeConference Objecten_US
dc.relation.conferenceNational Conference of Serbian Astronomers (15 ; 2008 ; Belgrade)en_US
dc.relation.publicationProceedings of the 15th National Conference of Astronomers of Serbiaen_US
dc.identifier.urlhttps://publications.aob.rs/86/pdf/279-282.pdf-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn0373-3742en_US
dc.description.rankM63en_US
dc.relation.firstpage279en_US
dc.relation.lastpage282en_US
dc.relation.issue86en_US
item.openairetypeConference Object-
item.languageiso639-1en-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-5139-1978-
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