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_US
dc.language.isoenen_US
dc.publisherOxford Academicen_US
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen_US
dc.subjectAtomic dataen_US
dc.subjectAtomic processesen_US
dc.subjectLine: formationen_US
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.isi000379832800040-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84983070086-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn0035-8711en_US
dc.description.rankM21en_US
dc.relation.firstpage1658en_US
dc.relation.lastpage1663en_US
dc.relation.volume460en_US
dc.relation.issue2en_US
item.openairetypeArticle-
item.fulltextNo Fulltext-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-5139-1978-
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