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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/963
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dc.contributor.authorDimitrijević, Milan S.en_US
dc.contributor.authorChristova, Magdalenaen_US
dc.contributor.authorSimić, Zoranen_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorSahal-Bréchot, Sylvieen_US
dc.date.accessioned2022-08-16T11:22:37Z-
dc.date.available2022-08-16T11:22:37Z-
dc.date.issued2012-01-01-
dc.identifier.isbn9781632662200-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/963-
dc.description.abstractThe preliminary results for Stark broadening parameters of B IV lines from 8 spectral series have been calculated using Sahal-Bréchot theory based on the semiclassical perturbation formalism.en
dc.titleOn the stark broadening of B IV spectral linesen_US
dc.typeConference Paperen_US
dc.relation.publicationVIII Serbian-Bulgarian Astronomical Conference, SBAC 2012en_US
dc.identifier.scopus2-s2.0-84902485309-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84902485309-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage205en_US
dc.relation.lastpage218en_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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