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Distribution and evolution of Li abundance in red clump stars can be explained by the internal gravity waves

Fuente: arXiv

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Bibliographic Details
Main Authors:	Li, Xuefeng, Shi, Jianrong, Li, Yan, Yan, Hongliang, Zhang, Jinghua
Format:	Preprint
Published:	2024
Subjects:	Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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