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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/3055
DC FieldValueLanguage
dc.contributor.authorPopović, Lukaen_US
dc.contributor.authorMediavilla, Een_US
dc.contributor.authorBon, Een_US
dc.contributor.authorIlić, Draganaen_US
dc.date.accessioned2026-01-12T13:29:42Z-
dc.date.available2026-01-12T13:29:42Z-
dc.date.issued2004-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/3055-
dc.description.abstractWe present a study of the emission line profiles of a sample of 12 single-peaked Active Galactic Nuclei (AGNs- Sy 1 and QSOs). The narrow [OIII] lines seem to be related to two components; NLR1, which has dispersion velocities from 200 to 500 km s−1 and is blueshifted with respect to the systemic by about 20 to 350 km s−1; and NLR2, with smaller dispersion velocities (∼100-200 km s−1) and a redshift corresponding to the cosmological one. The broad lines have complex structure and a two-component model has been applied.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.htmlen_US
dc.language.isoenen_US
dc.publisherCambridge : Cambridge University Pressen_US
dc.relation.ispartofProceedings of the International Astronomical Unionen_US
dc.titleEmission Line Region in a sample of 12 Active Galactic Nucleien_US
dc.typeConference Objecten_US
dc.relation.conferenceIAU Symposium The Interplay Among Black Holes, Stars and ISM in Galactic Nuclei (222 ; 2004 ; Gramado, Rio Grande do Sul)en_US
dc.relation.publicationThe Interplay Among Black Holes, Stars and ISM in Galactic Nucleien_US
dc.identifier.doi10.1017/S1743921304002583-
dc.identifier.urlhttp://dx.doi.org/10.1017/S1743921304002583-
dc.contributor.affiliationAstronomyen_US
dc.contributor.affiliationAstronomyen_US
dc.relation.issn1743-9213en_US
dc.description.rankM33en_US
dc.relation.firstpage355en_US
dc.relation.lastpage356en_US
dc.relation.volume2004en_US
dc.relation.issueIAUS222en_US
item.cerifentitytypePublications-
item.languageiso639-1en-
item.fulltextNo Fulltext-
item.openairetypeConference Object-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.deptAstronomy-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0003-2398-7664-
crisitem.author.orcid0000-0002-1134-4015-
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