Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/312
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dc.contributor.authorTapalaga, Irinelen
dc.contributor.authorTrklja, Noraen
dc.contributor.authorDojčinović, Ivanen
dc.contributor.authorPurić, Jagošen
dc.date.accessioned2022-07-12T15:09:05Z-
dc.date.available2022-07-12T15:09:05Z-
dc.date.issued2018-03-01en
dc.identifier.issn0035-8711en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/312-
dc.description.abstractStark width regularities within spectral series of the lithium isoelectronic sequence have been studied in an approach that includes both neutrals and ions. The influence of environmental conditions and certain atomic parameters on the Stark widths of spectral lines has been investigated. This study gives a simple model for the calculation of Stark broadening data for spectral lines within the lithium isoelectronic sequence. The proposed model requires fewer parameters than any other model. The obtained relations were used for predictions of Stark widths for transitions that have not yet been measured or calculated. In the framework of the present research, three algorithms for fast data processing have been made and they enable quality control and provide verification of the theoretically calculated results.en
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.subjectAtomic dataen
dc.subjectLine: profilesen
dc.subjectOpacityen
dc.subjectPlasmasen
dc.titleStark width regularities within spectral series of the lithium isoelectronic sequenceen
dc.typeArticleen
dc.identifier.doi10.1093/mnras/stx3114en
dc.identifier.scopus2-s2.0-85046084856en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85046084856en
dc.relation.issue4en
dc.relation.volume474en
dc.relation.firstpage5479en
dc.relation.lastpage5484en
item.grantfulltextnone-
item.openairetypeArticle-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
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