Asteroseismic rotation rates of hot subdwarf B stars hint at transient accretion from leftover common envelope matter

Fuente: arXiv

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Bibliographic Details
Main Authors:	Moyano, Facundo D., Ge, Hongwei, Han, Zhanwen, Bordadágua, Beatriz, Uzundag, Murat, Podsiadlowski, Philipp, Schaffenroth, Veronika, Chen, Xuefei, Liu, Zhengwei
Format:	Preprint
Published:	2026
Subjects:	Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2604.22233