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Fig. 3


Mass-loss rate and braking torque as functions of rotational velocity for stars of mass 0.5 M (black), 0.8 M (dark blue), and 1 M (light blue). Top panel: comparison between the mass-loss rate obtained with our model (solid curves) and the prescription of Cranmer & Saar (2011; dotted curves). Bottom panel: braking torque.

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