Stark broadening of Cd I spectral lines Virtual Observatory Resource

Authors
  1. Simic Z.
  2. Dimitrijevic M.S.
  3. Milovanovic N.
  4. Sahal-Brechot S.
  5. Published by
    CDS
Abstract

Stark broadening parameters, widths, and shifts for 33 CdI singlets and 37 triplets were calculated using the semiclassical perturbation method. The results were compared with available experimental and theoretical data. Also, regularity in the spectral series 5s^2^ ^1^S-np ^1^P^o^ was investigated. The influence of Stark broadening was analyzed in A-type stellar atmospheres.

Keywords
  1. Atomic physics
Bibliographic source Bibcode
2005A&A...441..391S
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/441/391
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/441/391
Document Object Identifer DOI
doi:10.26093/cds/vizier.34410391

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/441/391
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/441/391
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/441/391
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2005-10-22T12:47:47Z
Resource record created
2005-10-22T12:47:47Z
Created
2005-10-22T12:48:26Z
Updated

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