1. Research with MATF
  2. MATF
  3. Research outputs
Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/943
DC FieldValueLanguage
dc.contributor.authorSimić, Z.en_US
dc.contributor.authorDimitrijević, M. S.en_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorSahal-Bréchot, S.en_US
dc.date.accessioned2022-08-16T11:22:34Z-
dc.date.available2022-08-16T11:22:34Z-
dc.date.issued2011-01-01-
dc.identifier.issn13920049en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/943-
dc.description.abstractIn the deeper layers of hot stellar photospheres the Stark widths of spectral lines can be comparable and even larger than the thermal Doppler widths. Using the semiclassical perturbation method, we investigate the influence of the collisions with charged particles for the In III lines. We determine a number of Stark broadening parameters important in the atmospheres of A- type stars and white dwarfs. Also, the obtained results are compared with the available experimental data. The results will be included in the STARK- B database, the Virtual Atomic and Molecular Data Center and the Serbian Virtual Observatory.en
dc.relation.ispartofBaltic Astronomyen
dc.subjectSpectral linesen
dc.subjectStark broadeningen
dc.subjectStars: atmospheresen
dc.titleStark broadening of in III lines in astrophysical and laboratory plasmaen_US
dc.typeArticleen_US
dc.identifier.doi10.1515/astro-2017-0347-
dc.identifier.scopus2-s2.0-84855699650-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84855699650-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage613en
dc.relation.lastpage617en
dc.relation.volume20en
dc.relation.issue4en
item.fulltextNo Fulltext-
item.openairetypeArticle-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-5139-1978-
Appears in Collections:Research outputs
Show simple item record

SCOPUSTM   
Citations

2
checked on Nov 14, 2024

Page view(s)

11
checked on Nov 14, 2024

Google ScholarTM

Check

Altmetric

Altmetric


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.