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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/969
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dc.contributor.authorDimitrijević, Milan S.en_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorSimić, Zoranen_US
dc.contributor.authorDačič, Miodragen_US
dc.date.accessioned2022-08-16T11:22:38Z-
dc.date.available2022-08-16T11:22:38Z-
dc.date.issued2008-10-22-
dc.identifier.isbn9780735405714-
dc.identifier.issn0094243Xen
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/969-
dc.description.abstractThe Stark broadening parameters of O V 1371 Å spectral line, observed in stellar atmospheres of hot stars, determined within the semiclassical perturbation method, are used for the analysis of the importance of this broadening mechanism in white dwarf atmospheres. We found that Stark broadening mechanism is very important in such plasma conditions and should be taken into account. © 2008 American Institute of Physics.en
dc.relation.ispartofAIP Conference Proceedingsen_US
dc.subjectAtomic processesen
dc.subjectLine profilesen
dc.subjectStarsen
dc.subjectWhite dwarfen
dc.titleStark broadening of O v 1371 Å line in stellar atmospheresen_US
dc.typeConference Paperen_US
dc.relation.publicationExploring the Solar System and the Universe 2008en_US
dc.identifier.doi10.1063/1.2993686-
dc.identifier.scopus2-s2.0-54049128902-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/54049128902-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage410en_US
dc.relation.lastpage411en_US
dc.relation.volume1043en_US
item.fulltextNo Fulltext-
item.openairetypeConference Paper-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-5139-1978-
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