Formulating Mass-loss Rates for Sun-like Stars: A Hybrid Model Approach

Formulating Mass-loss Rates for Sun-like Stars: A Hybrid Model Approach

We observe an enhanced stellar wind mass-loss rate from low-mass stars exhibiting higher X-ray flux. This trend, however, does not align with the Sun, where no evident correlation between X-ray flux and mass-loss rate is present. To reconcile these observations, we propose a hybrid model for the ste...

Ausführliche Beschreibung

Bibliographische Detailangaben
Hauptverfasser:	Munehito Shoda, Steven R. Cranmer, Shin Toriumi
Format:	Artikel
Sprache:	English
Veröffentlicht:	IOP Publishing 2023-01-01
Schriftenreihe:	The Astrophysical Journal
Schlagworte:	Stellar winds Solar wind Magnetohydrodynamical simulations Alfven waves Solar magnetic reconnection
Online Zugang:	https://doi.org/10.3847/1538-4357/acfa72

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