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Fig. 3

image

Velocity profile as a function of radius for a set of 10 M stellar models with different mass-loss rates (as in Fig. 1). The black continuous lines indicate models with ≥ 2 × 10−5 M yr−1 (2, 3, 5 × 10−5), while the pink dashed lines indicate models with ≤ 1 × 10−5 M yr−1 (5, 8, 10 × 10−6). The green dashed line and the orange dot-dashed line indicate the local isothermal sound speed of the model with = 5 × 10−6 M yr−1 and the plane parallel grey atmosphere model with = 8 × 10−6 M yr−1, respectively.

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