Stark broadening of Ga I spectral lines

DOI

Stark broadening of the 18 Ga I transitions has been analyzed within the framework of the semiclassical perturbation method. Results obtained have been compared with available experimental and theoretical data and used for the consideration of the influence of the Stark broadening effect in stellar atmospheres

Identifier
DOI http://doi.org/10.26093/cds/vizier.34251147
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/425/1147
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/425/1147
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/425/1147
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/425/1147
Provenance
Creator Dimitrijevic M.S.; Dacic M.; Cvetkovic Z.; Simic Z.
Publisher CDS
Publication Year 2004
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Physics