CNO abundances in carbon stars Virtual Observatory Resource

Authors
  1. Ohnaka K.
  2. Tsuji T.
  3. Aoki W.
  4. Published by
    CDS
Abstract

The lines of ^12^CO, ^12^C^12^C, and ^12^CN used in the analysis are listed in the table. The stars analyzed here are TX Psc, V Aql, and BL Ori, and the lines selected for the analysis are listed for each star. The data given in the table are the wavenumber, gf-value, and the lower excitation potential of each selected line, together with the observed equivalent width.

Keywords
  1. carbon-stars
  2. chemical-abundances
  3. line-intensities
Bibliographic source Bibcode
2000A&A...353..528O
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/353/528
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/353/528
Document Object Identifer DOI
doi:10.26093/cds/vizier.33530528

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/353/528
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/353/528
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/353/528
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2000-01-29T18:08:30Z
Resource record created
2000-01-29T17:08:35Z
Updated
2000-01-29T18:08:30Z
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