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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/967
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dc.contributor.authorDimitrijević, Milan S.en_US
dc.contributor.authorSimić, Zoranen_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorSahal-Bréchot, Sylvieen_US
dc.date.accessioned2022-08-16T11:22:37Z-
dc.date.available2022-08-16T11:22:37Z-
dc.date.issued2018-01-01-
dc.identifier.issn10556796en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/967-
dc.description.abstractRecently, Stark broadening parameters have been calculated for a large number of Xe VIII spectral lines, for broadening by electron, proton, and He III impacts, using the impact semi-classical perturbation approach. The obtained results for 6s2S1/2–6p2Po1/2 transition have been used here to study the influence of Stark broadening on spectral lines in DO white dwarf atmospheres and the importance of Stark broadening due to collisions with electrons, protons and He III ions is shown.en
dc.relation.ispartofAstronomical and Astrophysical Transactionsen_US
dc.subjectAtomic dataen
dc.subjectDO white dwarfsen
dc.subjectStark broadenigen
dc.subjectXe VIIIen
dc.titleThe influence of stark broadening on xe VIII spectral lines in DO white dwarfsen_US
dc.typeArticleen_US
dc.identifier.scopus2-s2.0-85049592021-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85049592021-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage331en_US
dc.relation.lastpage336en_US
dc.relation.volume30en_US
dc.relation.issue3en_US
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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