Abundances of 94 stars Virtual Observatory Resource

Authors
  1. Nissen P.E.
  2. Schuster W.J.
  3. Published by
    CDS
Abstract

Abundances of Mn, Cu, Zn, Y, and Ba are determined for a sample of stars previously studied by Nissen & Schuster (2010, Cat. J/A+A/511/L10). Equivalent widths of atomic lines are measured from high resolution VLT/UVES and NOT/FIES spectra and used to derive abundance ratios from an LTE analysis based on MARCS model atmospheres. The analysis is made relative to two thick-disk stars, HD22879 and HD76932, such that very precise differential values are obtained.

Keywords
  1. Chemical abundances
  2. Line intensities
Bibliographic source Bibcode
2011A&A...530A..15N
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/530/A15
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/530/A15
Document Object Identifer DOI
doi:10.26093/cds/vizier.35300015

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/530/A15
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/530/A15
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/530/A15
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/A+A/530/A15/stars?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/530/A15/stars?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/530/A15/stars?

History

2011-04-28T13:01:35Z
Resource record created
2011-04-28T13:01:35Z
Created
2017-11-29T11:48:15Z
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