Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/973
DC FieldValueLanguage
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.accessioned2022-08-16T11:22:38Z-
dc.date.available2022-08-16T11:22:38Z-
dc.date.issued2010-01-01-
dc.identifier.isbn9781632662194-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/973-
dc.description.abstractIn order to provide Stark broadening data in X-ray and far UV wavelength region, of interest for modelling and analysis of astrophysical plasmas in extreme conditions, we performed calculations of Stark broadened line widths and shifts for Ar XV using the semiclassical perturbation theory.en_US
dc.language.isoenen_US
dc.publisherBeograd : Astronomsko društvo "Ruđer Bošković"en_US
dc.relation.ispartofPublikacije astronomskog društva "Rudjer Bošković"en_US
dc.titleOn the stark broadening of Ar XV spectral linesen_US
dc.typeConference Objecten_US
dc.relation.conferenceSerbian-Bulgarian Astronomical Conference SBAC (7 ; 2010 ; Chepelare)en_US
dc.relation.publicationVII Serbian-Bulgarian Astronomical Conference, SBAC 2010en_US
dc.identifier.scopus2-s2.0-84902449072-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84902449072-
dc.contributor.affiliationAstronomyen_US
dc.description.rankM33en_US
dc.relation.firstpage243en_US
dc.relation.lastpage246en_US
dc.relation.volume11en_US
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.grantfulltextnone-
item.openairetypeConference Object-
item.languageiso639-1en-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-5139-1978-
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