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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/941
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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.accessioned2022-08-16T11:22:34Z-
dc.date.available2022-08-16T11:22:34Z-
dc.date.issued2011-12-01-
dc.identifier.issn13920049en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/941-
dc.description.abstractIn order to complete Stark broadening data for Ne II and O III lines, needed for analysis of stellar atmospheres, we determined the missing parameters for the broadening by collisions with protons and ionized helium for 15 Ne II and 5 O III multiplets. Also, electron, proton and ionized helium impact broadening parameters for an important Nell multiplet in the visible part of the spectrum and for three Ne III multiplets were calculated. The obtained data will be included in 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 Nell, Ne III and Olli spectral lines for the Stark-B databaseen_US
dc.typeArticleen_US
dc.identifier.scopus2-s2.0-84855669443-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84855669443-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage580en
dc.relation.lastpage586en
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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