(Top) Mean Hα profile of BF Ori from the October campaign in Paper I (solid line) and magnetospheric accretion synthetic profile that best reproduces it (dashed line; M_∗ = 2.5 M_⊙, R_∗ = 2.5 R_⊙, T_∗ = 9000 K, magnetosphere size 4.2–5 R_∗, Ṁ_acc = 10^-8 M_⊙ yr^-1, i = 75 deg, and vsini = 37 km s^-1). The dotted line is the same synthetic profile with no rotation. (Bottom) Magnetospheric accretion synthetic Hα profiles with a stellar rotation rate of 75 km s^-1 (dashed lines) and with no rotation (dotted lines).