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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/937
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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.accessioned2022-08-16T11:22:33Z-
dc.date.available2022-08-16T11:22:33Z-
dc.date.issued2016-08-01-
dc.identifier.issn00358711en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/937-
dc.description.abstractStark broadening parameters for 157 multiplets of helium-like boron (B iv) have been calculated using the impact semiclassical perturbation formalism. Obtained results have been used to investigate the regularities within spectral series. An example of the influence of Stark broadening on B iv lines in DO white dwarfs is given.en
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.subjectAtomic dataen
dc.subjectAtomic processesen
dc.subjectLine: formationen
dc.titleStark broadening of B IV spectral linesen_US
dc.typeArticleen_US
dc.identifier.doi10.1093/mnras/stw1023-
dc.identifier.scopus2-s2.0-84983070086-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84983070086-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage1658en
dc.relation.lastpage1663en
dc.relation.volume460en
dc.relation.issue2en
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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