Fig. 10.

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Torques by the stellar wind (expressed in units of J⋆) in dependence of the stellar rotation rate in the cases without magnetospheric ejection (αm = 0.4, 0.7, 1.0). With the square, circle and triangle symbols are plotted approximate matching functions, indicated in each panel. In most of the cases,
is increasingly negative with the increase in stellar magnetic field strength and rotation rate. The cases with slower stellar rotation often do not match the approximated functions.
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