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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/3070
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dc.contributor.authorDimitrijevic, Milan Sen_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorSimic, Zoran Jen_US
dc.contributor.authorDacic, Miodrag Den_US
dc.date.accessioned2026-01-14T10:21:04Z-
dc.date.available2026-01-14T10:21:04Z-
dc.date.issued2008-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/3070-
dc.description.abstractThe Stark broadening parameters of 0 V 1371 angstrom 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.en_US
dc.language.isoenen_US
dc.publisherAIP Publishingen_US
dc.relation.ispartofAIP Conference Proceedingsen_US
dc.titleStark broadening of O V 1371 angstrom line in stellar atmospheresen_US
dc.typeConference Objecten_US
dc.relation.conferenceInternational Conference on Exploring the Solar System and the Universe (2008 ; Bucharest)en_US
dc.relation.publicationExploring the Solar System and the Universeen_US
dc.identifier.isi000259605500083-
dc.relation.issn0094-243Xen_US
dc.description.rankM34en_US
dc.relation.firstpage410en_US
dc.relation.lastpage410en_US
dc.relation.volume1043en_US
item.openairetypeConference Object-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextnone-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-5139-1978-
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