Fig. B.1.
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Comparison of the APSW torque formulation used in this study, ΓW (Eq. B.1), with that in Gallet et al. (2019), ΓW, G19, for a range of accretion rates. In addition, the value of Rt/Rco is shown. The stellar parameters are Ṁ⋆ = 0.7 M⊙, B⋆ = 0.5 kG, P⋆ = 2 days, and τage = 2 Myr. The horizontal line separates the regions in which the respective wind models produce stronger torques.
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