HE 1327−2326, an Unevolved Star with [Fe/H]<−5.0. II. New 3D−1D Corrected Abundances from a Very Large Telescope UVES Spectrum-Reference-Cited by-同舟云学术

HE 1327−2326, an Unevolved Star with [Fe/H]<−5.0. II. New 3D−1D Corrected Abundances from a Very Large Telescope UVES Spectrum

Published:2008-09 Issue:1 Volume:684 Page:588-602
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:Astrophysical Journal

Author:

Frebel Anna,Collet Remo,Eriksson Kjell,Christlieb Norbert,Aoki Wako

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference49 articles.

1. Spectroscopic Studies of Very Metal‐poor Stars with the Subaru High Dispersion Spectrograph. III. Light Neutron‐Capture Elements

2. HE 1327−2326, an Unevolved Star with [Fe/H] < −5.0. I. A Comprehensive Abundance Analysis

3. New Light on Stellar Abundance Analyses: Departures from LTE and Homogeneity

4. On OH line formation and oxygen abundances in metal-poor stars

5. Asplund, M., Grevesse, N. & Sauval, A. J. 2005, in ASP Conf. Ser. 336, Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis, ed. T. G. Barnes III & F. N. Bash (San Francisco: ASP), 25

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