The Angular Momentum of Stars Reflects the Relationship between Star-forming Environment and Galactic Evolution History

This study focuses on stars with masses above the Kraft break in the Kepler field. Their rotational angular momenta are essentially the same as those at the zero-age main sequence. The angular momentum dissipation experienced by these stars during their pre-main sequence (PMS) phase is also relative...

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Bibliographic Details
Main Authors: Yu-Fu Shen, Yan Xu, Yi-Bo Wang, Xiu-Lin Huang, Xing-Xing Hu, Qi Yuan
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/ade399
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