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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 7.

Same as Figure 3, for the Proxima Cen stellar parameters and δ v ⋆ = 5 km s−1 and λ ⋆ = 0.01R ⋆. The mass-loss rate of the simulation is at the upper bound ﹩\dot{M}=0.17{\dot{M}}_{\odot }﹩. The semimajor axis of Proxima Cen b is shown in red, within or very close to the (fast) Alfvén surface of the stellar wind.

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