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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/3027
DC FieldValueLanguage
dc.contributor.authorIlić, Draganaen_US
dc.date.accessioned2026-01-09T11:57:07Z-
dc.date.available2026-01-09T11:57:07Z-
dc.date.issued2009-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/3027-
dc.description.abstractActive Galactic Nuclei (AGN) are among the most spectacular objects in the sky since they produce enormous amounts of energy in a tiny volume, having luminosities of L ≈ 1042 – 1048 erg s−1. AGN emit in the continuum, as well as in the spectral lines, from γ and X-ray to the far infrared and radio domain. Their emission lines can be classified as narrow (NELs) or broad emission lines (BELs) according to their widths, and they are formed in two different emission regions, the narrow line region (NLR) and broad line region (BLR)en_US
dc.language.isoenen_US
dc.publisherBeograd : Astronomska opservatorijaen_US
dc.relation.ispartofPublications of Astronomical Observatory of Belgradeen_US
dc.titleKinematical and Physical Properties of the Central Emission Regions of Active Galaxy Mrk 817en_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, 2009,en_US
dc.identifier.isi000291668000068-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn0373-3742en_US
dc.description.rankM63en_US
dc.relation.firstpage405en_US
dc.relation.lastpage406en_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.orcid0000-0002-1134-4015-
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