Metal-poor field stars abundances

DOI

We have determined Li, C, N, O, Na, and Fe abundances, and ^12^C/^13^C isotopic ratios for a sample of 62 field metal-poor stars in the metallicity range -2<=[Fe/H]<=-1. Stars were selected in order to have accurate luminosity estimates from the literature, so that evolutionary phases could be clearly determined for each star. We further enlarged this dataset by adding 43 more stars having accurate abundances for some of these elements and similarly well defined luminosities from the literature.

Cone search capability for table J/A+A/354/169/table1 (Basic data for the programme star)

Identifier
DOI http://doi.org/10.26093/cds/vizier.33540169
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/354/169
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/354/169
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/354/169
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/354/169
Provenance
Creator Gratton R.G.; Sneden C.; Carretta E.; Bragaglia A.
Publisher CDS
Publication Year 2000
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