The SAM after the disk phase j_final as a function of stellar magnetic field values (x-axis and colors) and for different initial rotation periods (different sets of point styles and curves). Each panel shows the variation of one parameter with respect to the reference case in Fig. 7. In panel a, Ṁ_low is used as the initial accretion rate. In panels b and c, the APSW efficiency is set to 0% and 5%, respectively. In panel d, the viscous α parameter is set to 0.005. In all cases, the stellar mass is 0.3 M_⊙. The symbols and lines are identical to Fig. 7. For comparison, the yellow lines show the fits from Fig. 7 for a stellar mass of 0.3 M_⊙.