Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/3047
DC FieldValueLanguage
dc.contributor.authorIlić, Draganaen_US
dc.contributor.authorBon, Edien_US
dc.contributor.authorMediavilla, E Gen_US
dc.contributor.authorPopović, Lukaen_US
dc.date.accessioned2026-01-11T18:30:53Z-
dc.date.available2026-01-11T18:30:53Z-
dc.date.issued2003-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/3047-
dc.description.abstractThe analysis of emission line region of Seyfert 1 galaxy Mrk817 is presented. We found that emission line region in Mrk 817 is very complex. Moreover, the Narrow Line Region shows complex structure. The spectral line shapes of Mrk 817 indicates at least three kinematically separated regions, one (or more) which emits the broad line component (V ∼ 5000 km/s), one which emits narrow components (V ∼ 450 km/s) and one extensive which emits also narrow component (V ∼ 150 km/s).en_US
dc.language.isoenen_US
dc.publisherBeograd : Astronomska opservatorijaen_US
dc.relation.ispartofPublications de l'Observatoire Astronomique de Belgradeen_US
dc.titleThe emission line shapes of the Seyfert 1 galaxy Mrk 817en_US
dc.typeConference Objecten_US
dc.relation.conferenceSerbian Conference on Spectral Line Shapes (4 ; 2003 ; Belgrade)en_US
dc.relation.publicationIV Serbian Conference on Spectral Line Shapesen_US
dc.identifier.urlhttps://publications.aob.rs/76/pdf/197-200.pdf-
dc.contributor.affiliationAstronomyen_US
dc.contributor.affiliationAstronomyen_US
dc.relation.issn0373-3742en_US
dc.description.rankM63en_US
dc.relation.firstpage197en_US
dc.relation.lastpage200en_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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