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dc.creatorDimitrijević, Milan S.
dc.creatorSimić, Zoran
dc.creatorKovačević, Anđelka
dc.creatorValjarević, Aleksandar
dc.creatorSahal-Brechot, Sylvie
dc.date.accessioned2021-09-24T15:33:24Z
dc.date.available2021-09-24T15:33:24Z
dc.date.issued2015
dc.identifier.issn0250-6335
dc.identifier.urihttps://gery.gef.bg.ac.rs/handle/123456789/728
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.publisherIndian Acad Sciences, Bangalore
dc.relationinfo:eu-repo/grantAgreement/MESTD/Basic Research (BR or ON)/176002/RS//
dc.relationParis Observatory
dc.relationCentre National de la Recherche Scientifique (CNRS) - European Commission
dc.relationPNPS (Programme National de Physique Stellaire, INSU-CNRS)
dc.relationInvestissements d'avenir, French National Research Agency (ANR) [ANR-11-IDEX-0004-02]
dc.rightsrestrictedAccess
dc.sourceJournal of Astrophysics and Astronomy
dc.subjectStark broadeningen
dc.subjectatomic dataen
dc.subjectwhite dwarfsen
dc.subjectXe VIen
dc.titleStark Broadening in Compact Stars: Xe VI Linesen
dc.typeconferenceObject
dc.rights.licenseARR
dcterms.abstractДимитријевић, Милан С.; Ваљаревић, Aлександар; Сахал-Брецхот, Сyлвие; Ковачевић, Aнђелка; Симић, Зоран;
dc.citation.volume36
dc.citation.issue4
dc.citation.spage681
dc.citation.epage691
dc.citation.other36(4): 681-691
dc.citation.rankM23
dc.identifier.wos000368698700023
dc.identifier.doi10.1007/s12036-015-9352-y
dc.identifier.scopus2-s2.0-84956613605
dc.identifier.rcubhttps://hdl.handle.net/21.15107/rcub_gery_728
dc.type.versionpublishedVersion


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