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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/972
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dc.contributor.authorDimitrijević, Milan S.en_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorSimić, Zoranen_US
dc.contributor.authorSahal-Bréchot, Sylvieen_US
dc.date.accessioned2022-08-16T11:22:38Z-
dc.date.available2022-08-16T11:22:38Z-
dc.date.issued2011-01-01-
dc.identifier.issn13920049en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/972-
dc.description.abstractIn order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we determined Stark widths and shifts due to electron, proton and ionized helium impacts for nine lines (4191.0, 4259.4, 5912.1, 6043.2, 6045.0, 6752.9, 7503.9, 7514.6, 7724.2 A•), using jK coupling and semiclassical perturbation theory. The obtained results will enter the STARK-B database, which is a part of the Virtual Atomic and Molecular Data Center.en
dc.relation.ispartofBaltic Astronomyen
dc.subjectDatabasesen
dc.subjectLine profilesen
dc.subjectPhysical data and processes: Stark broadeningen
dc.titleStark broadening of several Ar I spectral lines in the visible Spectrumen_US
dc.typeArticleen_US
dc.identifier.doi10.1515/astro-2017-0339-
dc.identifier.scopus2-s2.0-84855705698-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84855705698-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage576en
dc.relation.lastpage579en
dc.relation.volume20en
dc.relation.issue4en
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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