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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/943
DC FieldValueLanguage
dc.contributor.authorSimić, Z.en_US
dc.contributor.authorDimitrijević, M. S.en_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorSahal-Bréchot, S.en_US
dc.date.accessioned2022-08-16T11:22:34Z-
dc.date.available2022-08-16T11:22:34Z-
dc.date.issued2011-01-01-
dc.identifier.issn13920049en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/943-
dc.description.abstractIn the deeper layers of hot stellar photospheres the Stark widths of spectral lines can be comparable and even larger than the thermal Doppler widths. Using the semiclassical perturbation method, we investigate the influence of the collisions with charged particles for the In III lines. We determine a number of Stark broadening parameters important in the atmospheres of A- type stars and white dwarfs. Also, the obtained results are compared with the available experimental data. The results will be included in the STARK- B database, the Virtual Atomic and Molecular Data Center and the Serbian Virtual Observatory.en_US
dc.language.isoenen_US
dc.publisherVilnus : University of Vilnusen_US
dc.relation.ispartofBaltic Astronomyen_US
dc.subjectSpectral linesen_US
dc.subjectStark broadeningen_US
dc.subjectStars: atmospheresen_US
dc.titleStark broadening of in III lines in astrophysical and laboratory plasmaen_US
dc.typeArticleen_US
dc.identifier.doi10.1515/astro-2017-0347-
dc.identifier.scopus2-s2.0-84855699650-
dc.identifier.isi000298717300021-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84855699650-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn1392-0049en_US
dc.description.rankM22en_US
dc.relation.firstpage613en_US
dc.relation.lastpage617en_US
dc.relation.volume20en_US
dc.relation.issue4en_US
item.openairetypeArticle-
item.languageiso639-1en-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-5139-1978-
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