Equivalent widths of 14 red giants Virtual Observatory Resource

Authors
  1. Pakhomov
  2. Yu.V.
  3. Published by
    CDS
Abstract

The results of a comparative analysis of the elemental abundances in the atmospheres of 14 red giants with high Galactic space velocities are presented. For almost all of the chemical elements considered, the their abundance trends with metallicity correspond to those constructed for thick-disk dwarfs. In the case of sodium, the main factor affecting the [Na/Fe] abundance in the stellar atmosphere for red giants is the surface gravity that characterizes the degree of development of the convective envelope. The difference between the [Na/Fe] abundances in the atmospheres of thin- and thick-disk red giants has been confirmed.

Keywords
  1. Giant stars
  2. Spectroscopy
  3. Line intensities
Bibliographic source Bibcode
2012PAZh...38..122P
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PAZh/38/122
IVOA Identifier IVOID
ivo://CDS.VizieR/J/PAZh/38/122

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PAZh/38/122
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PAZh/38/122
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PAZh/38/122
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/PAZh/38/122/stars?
https://vizier.iucaa.in/viz-bin/conesearch/J/PAZh/38/122/stars?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/PAZh/38/122/stars?

History

2013-12-11T12:20:52Z
Resource record created
2013-12-11T12:20:52Z
Created
2017-10-18T08:24:10Z
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