Torques by the stellar wind, (expressed in units of J_⋆) in terms of the dependence of the stellar rotation rate in the cases with the magnetospheric ejection, α_m = 0.1, (left). In all the cases except for the slowest stellar rotation rates, drops with dependence. is increasingly negative with the increase in stellar magnetic field strength and rotation rate, and is also decreasing slightly with 1/α_m (middle). Mass fluxes in the stellar wind in the cases with the fastest stellar rotation rates in our simulations (right) also mostly decrease slightly with 1/α_m. The y-label multiplication factor is given in the left upper corner of this panel.