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Magnetized Winds of M-type Stars and Star–Planet Magnetic Interactions: Uncertainties and Modeling Strategy

  • Authors: Victor Réville, Jamie M. Jasinski, Marco Velli, Antoine Strugarek, Allan Sacha Brun, Neil Murphy, Leonardo H. Regoli, Alexis P. Rouillard, Jacobo Varela

Victor Réville et al 2024 The Astrophysical Journal 976 .

  • Provider: AAS Journals

Caption: Figure 1.

The B. E. Wood et al. (2021) ﹩\dot{M}-{F}_{X}﹩ law with updated measurements from M dwarfs and slingshot prominences. The blue line represents the fitted law (Equation (1)). The dashed lines, one-tenth and 10 times the fitted law, encompass most of the 36 data points, with only a few outliers on the subgiant/giant branch. The filled regions in red and gray correspond to the mass-loss rate estimates for TRAPPIST-1 and Proxima Cen, respectively. The black cross symbol is the upper bound for Proxima Cen (all down arrows represent upper bounds).

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