Torques on the star in the simulation b16 (which is the DC case), with the same strength of magnetic field, 500 G as in the simulations b5 and b8, but with a star rotating two times faster. In this case, stellar rotation will be slowed down by the torque, because more of the torque comes from the disk beyond the corotation radius R_cor. The meanings behind the lines are the same as in the previous figure.