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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_US
dc.language.isoenen_US
dc.publisherDe Gruyteren_US
dc.relation.ispartofBaltic Astronomyen_US
dc.subjectDatabasesen_US
dc.subjectLine profilesen_US
dc.subjectPhysical data and processes: Stark broadeningen_US
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.isi000298717300013-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84855705698-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn1392-0049en_US
dc.description.rankM22en_US
dc.relation.firstpage576en_US
dc.relation.lastpage579en_US
dc.relation.volume20en_US
dc.relation.issue4en_US
item.openairetypeArticle-
item.fulltextNo Fulltext-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-5139-1978-
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