Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/55
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dc.contributor.authorDojčinović, Ivanen
dc.contributor.authorTapalaga, I.en
dc.contributor.authorPurić, J.en
dc.date.accessioned2022-06-30T14:05:50Z-
dc.date.available2022-06-30T14:05:50Z-
dc.date.issued2011-01-01en
dc.identifier.issn1323-3580en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/55-
dc.description.abstractThe dependences of Stark width on the upper-level ionization potential within different series of the neutral beryllium spectral lines have been studied. The dependences previously observed for electron impact contribution to the Stark widths were also obtained for the proton impact contribution. The emphasis is on the fine structure influence on the studied Stark parameter dependences. The influence of temperature on the dependences of Stark width parameters has been demonstrated. The relations found can be used in both cases for prediction of new Stark broadening data, thus avoiding much more complicated procedures. © 2011 Astronomical Society of Australia.en
dc.relation.ispartofPublications of the Astronomical Society of Australiaen
dc.subjectatomic dataen
dc.subjectline: profilesen
dc.subjectopacityen
dc.subjectplasmasen
dc.subjectradiative transferen
dc.titleStark width regularities within beryllium spectral seriesen
dc.typeArticleen
dc.identifier.doi10.1071/AS11014en
dc.identifier.scopus2-s2.0-82655166416en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/82655166416en
dc.relation.issue4en
dc.relation.volume28en
dc.relation.firstpage281en
dc.relation.lastpage289en
item.openairetypeArticle-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
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