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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 6.

Extent of the fast Alfvén surface as a function of δ v . Gray regions mark the minimum value of the fast Alfvén surface. Colored shades show its latitudinal variability for both values of λ . Horizontal black lines represent the semimajor axis of the first six planets of the TRAPPIST-1 system. For all simulations, at least one planet is within the maximal fast Alfvén radius, and can thus give birth to star–planet interactions. The dashed black line is the semimajor axis of Proxima Cen b in stellar radii.

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