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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 3.

Summary of four cases with the radial velocity, logarithm of temperature, radial Alfvén speed (﹩{B}_{r}/\sqrt{4\pi \rho }﹩), and velocity perturbation δ v. The (fast) Alfvén surface is shown in (dashed) white on top of each panel, while open (closed) magnetic field lines are shown in black (red). The δ v color scale varies for cases with different λ ⋆.

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