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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/959
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dc.contributor.authorDimitrijević, Milan S.en_US
dc.contributor.authorSimić, Zoranen_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorValjarević, Aleksandaren_US
dc.contributor.authorSahal-Bréchot, Sylvieen_US
dc.date.accessioned2022-08-16T11:22:36Z-
dc.date.available2022-08-16T11:22:36Z-
dc.date.issued2015-12-01-
dc.identifier.issn02506335en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/959-
dc.description.abstractWe will consider Stark broadening of non hydrogenic spectral lines in the impact approximation in compact stars: pre-white dwarf and white dwarf atmospheres. In order to show an example, Stark broadening parameters have been calculated, using the impact semiclassical perturbation approach for four Xe VI spectral lines. Obtained results have been used to demonstrate the influence of Stark broadening in DA and DB white dwarf atmospheres.en
dc.relation.ispartofJournal of Astrophysics and Astronomyen
dc.subjectatomic dataen
dc.subjectStark broadeningen
dc.subjectwhite dwarfsen
dc.subjectXe VIen
dc.titleStark Broadening in Compact Stars: Xe VI Linesen_US
dc.typeTexten_US
dc.identifier.doi10.1007/s12036-015-9352-y-
dc.identifier.scopus2-s2.0-84956613605-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84956613605-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage681en
dc.relation.lastpage691en
dc.relation.volume36en
dc.relation.issue4en
item.fulltextNo Fulltext-
item.openairetypeText-
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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