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The Oxygen Abundance of HE 1327-2326

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Authors

Frebel, Anna
Christlieb, Norbert
Norris, John
Aoki, Wako
Asplund, Martin

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IOP Publishing

Abstract

From a newly obtained VLT/UVES spectrum, we have determined the oxygen abundance of HE 1327-2326, the most iron-poor star known to date. Ultraviolet OH lines yield one-dimensional LTE abundances of [O/Fe]OH = 3.7 (subgiant case) and [O/Fe]OH = 3.4 (dwarf

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Source

Astrophysical Journal, The

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Restricted until

2037-12-31