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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_US
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.relation.ispartofJournal of Astrophysics and Astronomyen_US
dc.subjectatomic dataen_US
dc.subjectStark broadeningen_US
dc.subjectwhite dwarfsen_US
dc.subjectXe VIen_US
dc.titleStark Broadening in Compact Stars: Xe VI Linesen_US
dc.typeArticleen_US
dc.identifier.doi10.1007/s12036-015-9352-y-
dc.identifier.scopus2-s2.0-84956613605-
dc.identifier.isi000368698700023-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84956613605-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn0973-7758en_US
dc.description.rankM23en_US
dc.relation.firstpage681en_US
dc.relation.lastpage691en_US
dc.relation.volume36en_US
dc.relation.issue4en_US
item.grantfulltextnone-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairetypeArticle-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-5139-1978-
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