Torques, , (expressed in units of J_⋆) exerted on the star by material infalling from the disk in all the cases without magnetospheric ejection: these are all the cases except a,b,c,d(1,5,9,13), with the resistive coefficient α_m = 0.4, 0.7 and 1.0. Approximate matching functions and trends in solutions with different stellar rotation rates and magnetic field strengths are shown as (top) and (bottom). The dependence on α_m is small.