Positions of the anchoring radius, R_out, for the furthest stellar magnetic field line in the disk that still reaches the star and the inner disk radius, R_in. Top panels: R_out increases with the increasing resistive coefficient α_m for all stellar magnetic fields (left) and position of the R_out as a function of stellar rotation rate in the cases without magnetospheric ejection shows a decreasing trend with the stellar magnetic field (right). It is only in the cases with B_⋆ = 0.5 kG that we obtain a departure from this trend, with the largest R_out at the slowest stellar rotation rate. Bottom panels: Inner disk radius, R_in, is increasing in the majority of the cases with same parameters as in the above panels for R_out.