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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/935
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dc.contributor.authorDimitrijević, Milan S.en_US
dc.contributor.authorSimić, Zoranen_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorDačIć, Miodragen_US
dc.contributor.authorSahal-BréChot, Sylvieen_US
dc.date.accessioned2022-08-16T11:22:33Z-
dc.date.available2022-08-16T11:22:33Z-
dc.date.issued2008-01-01-
dc.identifier.isbn9781632662187-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/935-
dc.description.abstractWe determined Stark widths and shifts for four Te I multiplets, of interest for modellisation, investigation and diagnostic of stellar plasma, by using the semiclassical perturbation method. Results were applied for the investigation of the influence of Stark broadening mechanism in ultraviolet, optical and infrared part of the spectrum of white dwarf star atmospheres.en
dc.relation.ispartofPublikacije astronomskog društva "Rudjer Bošković"en_US
dc.titleStark broadening of neutral tellurium spectral lines in white dwarf atmospheresen_US
dc.typeConference Paperen_US
dc.relation.publicationVI Serbian-Bulgarian Astronomical Conference, SBAC 2008en_US
dc.identifier.scopus2-s2.0-84902522204-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84902522204-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage311en_US
dc.relation.lastpage314en_US
dc.relation.volume9en_US
item.fulltextNo Fulltext-
item.openairetypeConference Paper-
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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