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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/952
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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
dc.relation.ispartofNew Astronomy Reviewsen
dc.subjectAtomic dataen
dc.subjectCr IIen
dc.subjectLine profilesen
dc.subjectStark broadeningen
dc.subjectStellar atmospheresen
dc.subjectTe Ien
dc.titleStark broadening of spectral lines in chemically peculiar stars: Te I lines and recent calculations for trace elementsen_US
dc.typeTexten_US
dc.identifier.doi10.1016/j.newar.2009.08.005-
dc.identifier.scopus2-s2.0-70449521452-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/70449521452-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage246en
dc.relation.lastpage251en
dc.relation.volume53en
dc.relation.issue7-10en
item.fulltextNo Fulltext-
item.openairetypeText-
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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