Oxygen abundances: new results from [O I] lines

C. Sneden, F. Primas
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引用次数: 11

Abstract

Abstract Supersolar oxygen-to-iron ratios are known to exist in nearly all metal-poor stars. But there is no general agreement on the magnitude of these relative overabundances. New high resolution spectra of evolved stars over a large metallicity range have been gathered, from which lines of [O I], Sc II, and Fe II have been measured. Abundance ratios [O/Sc] and [O/Fe], insensitive to most model atmospheric uncertainties, have been derived and correlated with overall metallicity. These ratios both are consistent with earlier studies of the [O I] lines in metal-poor stars: [O/Sc]≃[O/Fe]≃+0.4, with possibly a small upward trend with decreasing [Fe/H].
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氧丰度:来自[O - I]系的新结果
众所周知,在几乎所有金属贫乏的恒星中都存在超级太阳氧铁比。但是对于这些相对过剩的程度并没有普遍的共识。在很大的金属丰度范围内,已经收集了演化恒星的新的高分辨率光谱,从中测量了[O I], Sc II和Fe II谱线。丰度比[O/Sc]和[O/Fe]对大多数模式大气不确定性不敏感,已经推导出并与总体金属丰度相关。这些比值与早期研究的贫金属恒星的[O/Sc]≃[O/Fe]≃+0.4一致,并且随着[Fe/H]的降低可能有小幅上升的趋势。
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