Equivalent widths of 26 metal-poor stars Virtual Observatory Resource

Authors

1. Aoki W.
2. Beers T.C.
3. Christlieb N.
4. Norris J.E.
5. Ryan S.G.
6. Tsangarides S.

Published by

CDS

Abstract

The chemical compositions of 26 metal-poor stars that exhibit strong CH and/or C2 molecular bands are determined. Twenty-two stars in our sample satisfy our definition for carbon-enhanced metal-poor (CEMP) stars based on the carbon abundance ratio ([C/Fe]) and the evolutionary status. In addition, we measure Na abundances for nine known carbon-enhanced stars. Combining our new sample with the results of previous work, we investigate the abundance and evolutionary status of a total of 64 CEMP stars.

Keywords

1. chemically-peculiar-stars
2. spectroscopy
3. photometry

Bibliographic source Bibcode

2007ApJ...655..492A

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https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/655/492

IVOA Identifier IVOID

ivo://CDS.VizieR/J/ApJ/655/492

Document Object Identifer DOI

doi:10.26093/cds/vizier.16550492

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