Mass losses in the outflow and in the stellar wind, Ṁ_out and Ṁ_SW, and mass flux through the disk Ṁ_d in solutions with magnetospheric outflow (α_m = 0.1), in terms of the dependence of the stellar rotation rate (top) and of the strength of stellar magnetic field (middle). The mass flux onto the star Ṁ_⋆ is also shown (bottom). The values of Ṁ_out and Ṁ_d are computed at R = 12R_⋆, while Ṁ_SW and Ṁ_⋆ are computed at the stellar surface. For illustration, shown are examples of matching functions. Note: the y-label multiplication factor is given in the left upper corner of the panels.