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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/952
DC FieldValueLanguage
dc.contributor.authorSimić, Zoranen_US
dc.contributor.authorDimitrijević, Milan S.en_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.date.accessioned2022-08-16T11:22:36Z-
dc.date.available2022-08-16T11:22:36Z-
dc.date.issued2009-07-01-
dc.identifier.issn13876473en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/952-
dc.description.abstractWith the development of astronomical observations from space, spectral lines of trace elements can now be observed in stellar spectra with good resolution, and atomic data for such atoms and ions have an increasing significance. We review here work in Belgrade on the influence of Stark broadening of trace elements on stellar spectra and present new determinations of Stark broadening parameters of neutral tellurium. Also the corresponding Stark and Doppler widths are compared in atmospheres of A type stars. © 2009 Elsevier B.V. All rights reserved.en_US
dc.language.isoenen_US
dc.publisherElsevieren_US
dc.relation.ispartofNew Astronomy Reviewsen_US
dc.subjectAtomic dataen_US
dc.subjectCr IIen_US
dc.subjectLine profilesen_US
dc.subjectStark broadeningen_US
dc.subjectStellar atmospheresen_US
dc.subjectTe Ien_US
dc.titleStark broadening of spectral lines in chemically peculiar stars: Te I lines and recent calculations for trace elementsen_US
dc.typeArticleen_US
dc.identifier.doi10.1016/j.newar.2009.08.005-
dc.identifier.scopus2-s2.0-70449521452-
dc.identifier.isi000272763900024-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/70449521452-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn1387-6473en_US
dc.description.rankM22en_US
dc.relation.firstpage246en_US
dc.relation.lastpage251en_US
dc.relation.volume53en_US
dc.relation.issue7-10en_US
item.openairetypeArticle-
item.languageiso639-1en-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-5139-1978-
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