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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/109
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dc.contributor.authorKovačević, J.en_US
dc.contributor.authorIlić, Draganaen_US
dc.contributor.authorGavrilović, N.en_US
dc.contributor.authorPopović, L.en_US
dc.date.accessioned2022-08-06T15:18:35Z-
dc.date.available2022-08-06T15:18:35Z-
dc.date.issued2006-01-01-
dc.identifier.isbn9788680019338-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/109-
dc.description.abstractUsing Active Galactic Nuclei (AGNs) spectra collected from the latest data release Four (DR4) of the Sloan Digital Sky Survey (SDSS),we study the kinematical properties of the [OIII] λλ 4959, 5007 Å narrow emission lines. The sample was selected using the following criteria: (i) the redshift of AGNs isz < 0.79 and (ii) the signal to noise ratio is S/N > 35. The aim of this work is to investigate an asymmetry in the [OIII] lines that may indicate an outflow in the AGNs Narrow Line Region (NLR).en
dc.titleInvestigation of kinematics of the NLR from the SDSS AGN sampleen_US
dc.typeConference Paperen_US
dc.relation.publicationProceedings of the 5th Bulgarian-Serbian Conference on Astronomy and Space Science: Astronomy and Space Science, BSCASS 2006en_US
dc.identifier.scopus2-s2.0-84929090762-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84929090762-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage353en_US
dc.relation.lastpage355en_US
item.fulltextNo Fulltext-
item.openairetypeConference Paper-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-1134-4015-
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