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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/948
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dc.contributor.authorSimic, Zoranen_US
dc.contributor.authorDimitrijevic, Milan S.en_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorDacic, Miodragen_US
dc.date.accessioned2022-08-16T11:22:35Z-
dc.date.available2022-08-16T11:22:35Z-
dc.date.issued2008-01-01-
dc.identifier.isbn9781632662187-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/948-
dc.description.abstractIn this paper, we presented Stark broadening parameters for four Cr II 3d5-3d4 4p multiplets calculated by the semiclassical perturbation approach. The obtained Stark broadening parameters were applied to the analysis of Cr II line profiles in hot star spectra.en
dc.relation.ispartofPublikacije astronomskog društva "Rudjer Bošković"en_US
dc.titleOn the stark broadening of Cr II 3d<sup>5</sup>-3d<sup>4</sup> 4p spectral lines in hot star spectraen_US
dc.typeConference Paperen_US
dc.relation.publicationVI Serbian-Bulgarian Astronomical Conference, SBAC 2008en_US
dc.identifier.scopus2-s2.0-84902436489-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84902436489-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage421en_US
dc.relation.lastpage424en_US
dc.relation.volume9en_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.orcid0000-0001-5139-1978-
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