Image Details

Choose export citation format:

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 9.

Radiative losses (same as Figure 5), compared with the integral of the TRAPPIST-1 synthetic spectrum in the EUV–FUV range (10–121.7 nm) with the method of K. Namekata et al. (2023) and J. L. Linsky et al. (2014). Plain and dashed blue lines correspond to λ = 0.001R and λ = 0.01R , respectively. The red box identifies the parameter range compatible with Wood’s law’s mass-loss rate.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse