Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/2865
DC FieldValueLanguage
dc.contributor.authorDimitrijevic, Milan Sen_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorSimic, Zoran Jen_US
dc.contributor.authorSahal-Brechot, Sylvieen_US
dc.date.accessioned2025-11-01T12:53:00Z-
dc.date.available2025-11-01T12:53:00Z-
dc.date.issued2011-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/2865-
dc.description.abstractIn order to complete Stark broadening data for Ne II and O IIIlines, needed for analysis of stellar atmospheres, we determined the missingparameters for the broadening by collisions with protons and ionized helium for15 Ne II and 5 O III multiplets. Also, electron, proton and ionized helium impactbroadening parameters for an important Ne II multiplet in the visible part ofthe spectrum and for three Ne III multiplets were calculated. The obtaineddata will be included in the STARK-en_US
dc.language.isoenen_US
dc.publisherDe Gruyteren_US
dc.relation.ispartofBaltic Astronomyen_US
dc.titleStark Broadening of Several Ne Ii, Ne Iii and O Iii Spectral Lines for the Stark-B Databaseen_US
dc.typeArticleen_US
dc.identifier.doi10.1515/astro-2017-0340-
dc.identifier.isi000298717300014-
dc.identifier.urlhttp://dx.doi.org/10.1515/astro-2017-0340-
dc.relation.issn1392-0049en_US
dc.description.rankM22en_US
dc.relation.firstpage580en_US
dc.relation.lastpage586en_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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