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Nonlinear Alfvén Wave Model of Stellar Coronae and Winds from the Sun to M Dwarfs

  • Authors: Takahito Sakaue, and Kazunari Shibata

2021 The Astrophysical Journal Letters 906 L13.

  • Provider: AAS Journals

Caption: Figure 2.

Temporal variations of the stellar wind velocity (panel (a)) and temperature (panel (b)) in the case of M3.5 dwarf (r = 0.46r). The stellar wind velocity reaches around 900 km s−1. The transition layer appears in the temperature profile, dividing the lower-temperature chromosphere and 10 MK corona.

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