Stark broadening of Ga I spectral lines Virtual Observatory Resource

Authors
  1. Dimitrijevic M.S.
  2. Dacic M.
  3. Cvetkovic Z.
  4. Simic Z.
  5. Published by
    CDS
Abstract

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

Keywords
  1. Atomic physics
Bibliographic source Bibcode
2004A&A...425.1147D
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/425/1147
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/425/1147
Document Object Identifer DOI
doi:10.26093/cds/vizier.34251147

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/425/1147
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/425/1147
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/425/1147
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2004-12-11T21:44:01Z
Resource record created
2004-12-11T20:44:08Z
Updated
2004-12-11T21:44:01Z
Created

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr