New line-driven wind mass-loss rates for OB stars with metallicities down to $0.01\,Z_\odot$

Fuente: arXiv

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Bibliographic Details
Main Authors:	Krticka, Jiri, Kubat, Jiri, Krtickova, Iva
Format:	Preprint
Published:	2025
Subjects:	Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2508.21702