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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/3106
DC FieldValueLanguage
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorShapovalova, Alla Ien_US
dc.contributor.authorPopović, Lukaen_US
dc.contributor.authorBurenkov, Alexander Nen_US
dc.contributor.authorChavushyan, Vahram Hen_US
dc.date.accessioned2026-01-19T08:09:21Z-
dc.date.available2026-01-19T08:09:21Z-
dc.date.issued2009-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/3106-
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 of Astronomical Observatory of Belgradeen_US
dc.title1d and 2d Reverberation Mapping Applied on the H-beta Line of NGC 4151en_US
dc.typeConference Objecten_US
dc.relation.conferenceNational Conference of Astronomers of Serbia (15 ; 2008 ; Belgrade)en_US
dc.relation.publicationProceedings of the XV National Conference of Astronomers of Serbia, Belgrade, Serbia, 2008.en_US
dc.identifier.urlhttps://publications.aob.rs/86/pdf/279-282.pdf-
dc.contributor.affiliationAstronomyen_US
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.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.orcid0000-0001-5139-1978-
crisitem.author.orcid0000-0003-2398-7664-
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