On Convective Turnover Times and Dynamos in Low-mass Stars

The relationship between magnetic activity and Rossby number is one way through which stellar dynamos can be understood. Using measured rotation rates and X-ray to bolometric luminosity ratios of an ensemble of stars, we derive empirical convective turnover times based on recent observations and ree...

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Bibliografski detalji

Glavni autori:	Seth Gossage, Rocio Kiman, Kristina Monsch, Amber A. Medina, Jeremy J. Drake, Cecilia Garraffo, Yuxi(Lucy) Lu, Joshua D. Wing, Nicholas J. Wright
Format:	Artigo
Jezik:	Inglês
Izdano:	IOP Publishing 2025-01-01
Serija:	The Astrophysical Journal
Teme:	Stellar evolutionary models Stellar activity Stellar rotation Stellar convection envelopes Stellar magnetic fields
Online pristup:	https://doi.org/10.3847/1538-4357/adde4d
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