Abundances in gamma Sge Virtual Observatory Resource

Authors
  1. Boyarchuk A.A.
  2. Antipova L.I.
  3. Boyarchuk M.E.
  4. Savanov I.S.
  5. Published by
    CDS
Abstract

CCD spectra are used to analyse the abundances of chemical elements in the atmosphere of the MOIII giant gamma Sagittae. Its atmospheric atmospheric parameters were determined to be T(eff)=3970K, logg=1.3, and microturbulence v(t)=1.65km/s.

Keywords
  1. m-stars
  2. spectroscopy
  3. chemical-abundances
Bibliographic source Bibcode
1995AZh....72..864B
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/72/864
IVOA Identifier IVOID
ivo://CDS.VizieR/J/AZh/72/864

Access

Web browser access HTML
https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AZh/72/864
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AZh/72/864
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AZh/72/864
IVOA Table Access TAP
https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2001-08-22T21:09:50Z
Resource record created
2001-08-22T21:09:50Z
Created
2001-08-22T21:11:41Z
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