Abundances in the Sgr dSph Virtual Observatory Resource

Authors
  1. Bonifacio P.
  2. Sbordone L.
  3. Marconi G.
  4. Pasquini L.
  5. Hill V.
  6. Published by
    CDS
Abstract

We report on abundances of O, Mg, Si, Ca and Fe for 10 giants in the Sgr dwarf spheroidal derived from high resolution spectra obtained with UVES at the 8.2m Kueyen-VLT telescope. The iron abundance spans the range -0.8<~[Fe/H]<~0.0 and the dominant population is relatively metal-rich with [Fe/H]~-0.25.

Keywords
  1. stellar-populations
  2. chemically-peculiar-stars
  3. line-intensities
Bibliographic source Bibcode
2004A&A...414..503B
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/414/503
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/414/503
Document Object Identifer DOI
doi:10.26093/cds/vizier.34140503

Access

IVOA Table Access TAP
https://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).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/414/503/table3?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/414/503/table3?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/414/503/table3?

History

2004-04-03T21:45:33Z
Resource record created
2004-04-03T21:45:33Z
Created
2004-04-03T21:45:42Z
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