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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/2912
DC FieldValueLanguage
dc.contributor.authorPopović, Lukaen_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorŠapovalova, A.en_US
dc.contributor.authorIlić, Draganaen_US
dc.date.accessioned2025-11-14T16:46:53Z-
dc.date.available2025-11-14T16:46:53Z-
dc.date.issued2010-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/2912-
dc.description.abstractThe timing analysis of light curves of astrophysical objects could reveal characteristic timescales which in turn describe physics of these objects. We applied cross correlation analysis in order to find the timescale of the lag between the Hβ line and continuum using the observations from the long-term spectral monitoring.en_US
dc.language.isoenen_US
dc.publisherBeograd : Astronomska opservatorijaen_US
dc.relation.ispartofPublications of the Astronomical Observatory of Belgradeen_US
dc.titleTiming Analysis of Light Curves of 3C390.3en_US
dc.typeConference Objecten_US
dc.relation.conferenceSummer School and International Symposium on Physics of Ionized Gases (24 ; 2010 ; Donji Milanovac)en_US
dc.relation.publication24th Summer School and International Symposium on the Physics of Ionized Gasesen_US
dc.identifier.urlhttps://publications.aob.rs/89/pdf/363-366.pdf-
dc.contributor.affiliationAstronomyen_US
dc.contributor.affiliationAstronomyen_US
dc.description.rankM33en_US
dc.relation.firstpage363en_US
dc.relation.lastpage366en_US
dc.relation.issue89en_US
item.openairetypeConference Object-
item.fulltextNo Fulltext-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.deptAstronomy-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-5139-1978-
crisitem.author.orcid0000-0002-1134-4015-
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