The radius variations of accreting main sequence stars and mass transfer instability

Fuente: arXiv

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Bibliographic Details
Main Authors:	Zhao, Zi-Qi, Li, Zhen-Wei, Xiao, Lin, Ge, Hong-Wei, Han, Zhan-Wen
Format:	Preprint
Published:	2024
Subjects:	Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2404.06148