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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/955
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dc.contributor.authorDimitrijević, M. S.en_US
dc.contributor.authorSimić, Z.en_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorDačić, M.en_US
dc.contributor.authorSahal-Bréchot, S.en_US
dc.date.accessioned2022-08-16T11:22:36Z-
dc.date.available2022-08-16T11:22:36Z-
dc.date.issued2008-04-01-
dc.identifier.issn13351842en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/955-
dc.description.abstractBy using the semiclassical perturbation method, Stark widths and shifts have been calculated for the Te I 6s 5So - 7p 5p (5125.2 Å) multiplet, of interest for CP star plasma studies. Results were applied to the investigation of the influence of Stark broadening on CP star spectra. It was found that layers exist in the stellar atmospheres considered where the Stark broadening contribution is comparable to or larger than the Doppler width.en
dc.relation.ispartofContributions of the Astronomical Observatory Skalnate Plesoen_US
dc.subjectAtomic dataen
dc.subjectAtomic processesen
dc.subjectLine: formationen
dc.subjectLine: profilesen
dc.subjectStars: atmospheresen
dc.subjectStars: chemically peculiaren
dc.titleOn the Stark broadening of Te I spectral lines for CP star plasma analysisen_US
dc.typeConference Paperen_US
dc.relation.publicationCP#AP workshop 2007en_US
dc.identifier.scopus2-s2.0-45749114184-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/45749114184-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage403en_US
dc.relation.lastpage404en_US
dc.relation.volume38en_US
dc.relation.issue2en_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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