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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/962
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dc.contributor.authorSimić, Z.en_US
dc.contributor.authorDimitrijević, M. S.en_US
dc.contributor.authorPopović, L. Čen_US
dc.contributor.authorDačić, M.en_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorSahal-Bréchot, S.en_US
dc.date.accessioned2022-08-16T11:22:37Z-
dc.date.available2022-08-16T11:22:37Z-
dc.date.issued2008-04-01-
dc.identifier.issn13351842en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/962-
dc.description.abstractStark broadening parameters for six Mn II lines are determined semi-classically and used to analyse the influence of this broadening mechanism on A-type star spectral line profiles. Results for the Mn II line at 2950.1 Å are presented here as an example of the data obtained.en
dc.relation.ispartofContributions of the Astronomical Observatory Skalnate Plesoen_US
dc.subjectAtomic dataen
dc.subjectLine profilesen
dc.subjectLine: formationen
dc.subjectStars: atmospheresen
dc.titleOn stark broadening of Mn II lines in Ap-star conditionsen_US
dc.typeConference Paperen_US
dc.relation.publicationCP#AP workshop 2007en_US
dc.identifier.scopus2-s2.0-45749154229-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/45749154229-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage451en_US
dc.relation.lastpage452en_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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