NGC 188 subgiant lithium abundances show a shallow temperature trend that favors rotationally induced mixing over mass loss or diffusion as the origin of the main-sequence lithium dip.
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Subgiants in NGC 188 Reveal that Rotationally Induced Mixing Creates the Main Sequence Li-Dip
NGC 188 subgiant lithium abundances show a shallow temperature trend that favors rotationally induced mixing over mass loss or diffusion as the origin of the main-sequence lithium dip.