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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/76
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dc.contributor.authorShapovalova, A. I.en_US
dc.contributor.authorPopović, L. Čen_US
dc.contributor.authorIlić, Draganaen_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorKovačević, J.en_US
dc.contributor.authorBurenkov, A. N.en_US
dc.contributor.authorChavushyan, V. H.en_US
dc.date.accessioned2022-08-06T15:18:31Z-
dc.date.available2022-08-06T15:18:31Z-
dc.date.issued2011-01-01-
dc.identifier.issn13920049en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/76-
dc.description.abstractWe present preliminary results of the long-term spectral monitoring of two active galactic nuclei with different broad line shapes: Ark 564 and Arp 102B. Ark 564 is a bright nearby narrow-line Syfert 1 (NLSl) galaxy with relatively narrow permitted optical emission lines and a high FeII/H/5 ratio, while Arp 102B is a nearby broad-line radio galaxy with broad double-peaked Balmer emission lines. The spectra of Ark 564 were observed during 11-year period (1999-2009) and the spectra of Arp 102B in the 12-year period (19982009), with SAO 6 m and 1 m telescopes (Russia) and the OAGH 2.1 m telescope (Cananea, Mexico).en
dc.relation.ispartofBaltic Astronomyen
dc.subjectArp 102b)en
dc.subjectGalaxies: Activeen
dc.subjectIndividual (ark 564en
dc.subjectSeyferten
dc.titleSpectral monitoring of AGN: Preliminary results for Ark 564 and Arp 102Ben_US
dc.typeConference Paperen_US
dc.identifier.doi10.1515/astro-2017-0323-
dc.identifier.scopus2-s2.0-84055216941-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84055216941-
dc.contributor.affiliationAstronomyen_US
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage476en
dc.relation.lastpage480en
dc.relation.volume20en
dc.relation.issue3en
item.fulltextNo Fulltext-
item.openairetypeConference Paper-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-1134-4015-
crisitem.author.orcid0000-0001-5139-1978-
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