Rotational velocities + Li abundance in K giants
收藏B2FIND2026-03-19 收录
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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)...
近轨道巨行星的轨道角动量可达到足够大的量级，以至于若在红巨星支（red giant branch, RGB）阶段将其转移至宿主恒星的包层中……
