G64-12 and G64-37 linelist and EWs
收藏B2FIND2026-03-19 收录
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https://b2find.eudat.eu/dataset/a99c0bb1-4456-50bd-991c-02bc6ba923ba
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Studies of extremely metal-poor stars indicate that chemical abundance ratios [X/Fe] have a root mean square scatter as low as 0.05dex (12%). It remains unclear whether this...
