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- W2318462137 abstract "Abstract The formation of [Oɪ], Oɪ and OH lines in metal-poor stars has been studied by means of 3D hydrodynamical model atmospheres. For Oɪ detailed 3D non-LTE calculations have been performed. While the influence of 3D model atmospheres is minor for [Oɪ] and Oɪ lines, the very low temperatures encountered at low metallicities have a drastic impact on OH. As a result, the derived O abundances are found to be systematically overestimated in 1D analyses, casting doubts on the recent claims for a monotonic increase in [O/Fe] towards lower metallicities." @default.
- W2318462137 created "2016-06-24" @default.
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- W2318462137 date "2002-01-01" @default.
- W2318462137 modified "2023-09-25" @default.
- W2318462137 title "Oxygen Line Formation in 3D Hydrodynamical Model Atmospheres" @default.
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- W2318462137 doi "https://doi.org/10.1017/s1539299600014003" @default.
- W2318462137 hasPublicationYear "2002" @default.
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