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- W1707718786 abstract "The formation of [O I], O I and OH lines in metal-poor stars has been studied by means of 3D hydrodynamical model atmospheres. For O I detailed 3D non-LTE calculations have been performed. While the influence of 3D model atmospheres is minor for [O I] and O I lines, the very low temperatures encountered at low metallicities have a drastic impact on the OH lines. 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.
- W1707718786 created "2016-06-24" @default.
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- W1707718786 date "2000-11-02" @default.
- W1707718786 modified "2023-09-27" @default.
- W1707718786 title "Oxygen line formation in 3D hydrodynamical model atmospheres" @default.
- W1707718786 hasPublicationYear "2000" @default.
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