Girish M. Duvvuri et al 2023 AJ 165 12
For low-mass stars, fast rotation is correlated with large-amplitude variability at optical wavelengths, which could be the result of heating by Alfvén waves or the result or small and frequent flares.
Girish M. Duvvuri et al 2023 AJ 165 12
For low-mass stars, fast rotation is correlated with large-amplitude variability at optical wavelengths, which could be the result of heating by Alfvén waves or the result or small and frequent flares.