Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/3003
DC FieldValueLanguage
dc.contributor.authorIlić, Draganaen_US
dc.contributor.authorPopović, Luka Čen_US
dc.contributor.authorBorka, Ven_US
dc.date.accessioned2025-12-12T18:43:20Z-
dc.date.available2025-12-12T18:43:20Z-
dc.date.issued2005-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/3003-
dc.description.abstractWe present a study on properties of ultraviolet spectra of a low red-shifted (with red-shift <0.4) sample of radio-loud and radio-quite active galactic nuclei (AGNs). The sample of galaxies was observed with the Hubble Space Telescope. We measured the ratios CIV1550/Lyα and NV/Lyα in order to see the similarities and differences in the UV emitting line region of radio-loud and radio-quite AGNs.en_US
dc.language.isoenen_US
dc.publisherItalian Astronomical Societyen_US
dc.relation.ispartofMemorie della Societa Astronomica Italianaen_US
dc.subjectquasarsen_US
dc.subjectUV emission linesen_US
dc.subjectbroad emission linesen_US
dc.titleThe UV spectral properties of radio loud and radio quiet QSOs: The ratio of NV/Lyalpha and CIV1550/Lyalphaen_US
dc.typeConference Objecten_US
dc.relation.conferenceMultiband Approach to AGN (2004 ; Bonn)en_US
dc.relation.publicationMultiband Approach to AGNen_US
dc.contributor.affiliationAstronomyen_US
dc.relation.issn0037-8720en_US
dc.description.rankM34en_US
dc.relation.firstpage51en_US
dc.relation.lastpage52en_US
dc.relation.volume76en_US
item.openairetypeConference Object-
item.languageiso639-1en-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-1134-4015-
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