Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/305
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dc.contributor.authorDojčinović, Ivanen
dc.contributor.authorTrklja, Noraen
dc.contributor.authorTapalaga, Irinelen
dc.contributor.authorPurić, Jagošen
dc.date.accessioned2022-07-12T15:09:03Z-
dc.date.available2022-07-12T15:09:03Z-
dc.date.issued2019-11-01en
dc.identifier.issn0035-8711en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/305-
dc.description.abstractWe have investigated Stark line broadening within the spectral series of potassium-like and copper-like emitters, both separately and together. The analysis was performed for fixed values of electronic density Ne = 1022 m-3 and temperature T = 100 000 K. Algorithms made for fast data processing also serve for temperature and density normalization of data. Relations obtained using the regularity-based analysis enable predictions of Stark widths for transitions that have not yet been calculated or measured. Results of present investigation can be used for quality control of available Stark width data.en
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.subjectAtomic dataen
dc.subjectGalaxies: Abundancesen
dc.subjectLine: Profilesen
dc.subjectOpacityen
dc.subjectPlasmasen
dc.titleInvestigation of Stark line broadening within spectral series of potassium and copper isoelectronic sequencesen
dc.typeArticleen
dc.identifier.doi10.1093/mnras/stz2367en
dc.identifier.scopus2-s2.0-85075171601en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85075171601en
dc.relation.issue3en
dc.relation.volume489en
dc.relation.firstpage2997en
dc.relation.lastpage3002en
item.openairetypeArticle-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
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