Atmospheric parameters in metal-poor stars. III. Virtual Observatory Resource

Authors

1. Carretta E.
2. Gratton R.G.
3. Sneden C.

Published by

CDS

Abstract

We present the results of the analysis of an extensive set of new and literature high quality data concerning Fe, C, N, O, Na, and Mg. This analysis exploited the T_eff_ scale determined in Gratton et al. (1996, Cat. <J/A+A/314/191>), and the non-LTE abundance corrections computed in Gratton et al. (1999, Cat. <J/A+A/350/955>). Results obtained with various abundance indices are discussed and compared.

Keywords

1. chemically-peculiar-stars
2. chemical-abundances

Bibliographic source Bibcode

2000A&A...356..238C

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ivo://CDS.VizieR/J/A+A/356/238

Document Object Identifer DOI

doi:10.26093/cds/vizier.33560238

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