Chemical abundances of 23 subgiants & giants

DOI

Chemical abundances, stellar parameters, and atomic and molecular line data are given for a study of 23 subgiant and giant stars in the solar vicinity. With the exception of Li and possibly C we show that subgiant stars show no "chemical" traces of post-main-sequence evolution and that they are therefore and because of their simple age dating very useful targets for studies of galactic chemical evolution.

Cone search capability for table J/A+A/425/187/table6 (Chemical abundances and stellar parameters)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34250187
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/425/187
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/425/187
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/425/187
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/425/187
Provenance
Creator Thoren P.; Edvardsson B.; Gustafsson B.
Publisher CDS
Publication Year 2004
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Physics; Stellar Astronomy