Rotational velocities + Li abundance in K giants
收藏B2FIND2026-03-19 收录
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https://b2find.eudat.eu/dataset/6fc9bdca-3923-5d1c-b879-f892ae45eb43
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The orbital angular momentum of a close-orbiting giant planet can be sufficiently large that, if transferred to the envelope of the host star during the red giant branch (RGB)...
