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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/970
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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.accessioned2022-08-16T11:22:38Z-
dc.date.available2022-08-16T11:22:38Z-
dc.date.issued2014-10-01-
dc.identifier.issn02731177en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/970-
dc.description.abstractStark broadening parameters for 36 multiplets of B IV have been calculated using the semi-classical perturbation formalism. Obtained results have been used to investigate the regularities within spectral series and temperature dependence. © 2014 Published by Elsevier Ltd.en
dc.relation.ispartofAdvances in Space Researchen
dc.subjectAtomic dataen
dc.subjectAtomic processesen
dc.subjectLine: profilesen
dc.subjectStars: atmospheresen
dc.titleStark broadening of B IV lines for astrophysical and laboratory plasma researchen_US
dc.typeArticleen_US
dc.identifier.doi10.1016/j.asr.2013.08.021-
dc.identifier.scopus2-s2.0-84906318625-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84906318625-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage1195en
dc.relation.lastpage1202en
dc.relation.volume54en
dc.relation.issue7en
item.fulltextNo Fulltext-
item.openairetypeArticle-
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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