Three different cases of geometry in the results. Top and middle panels: matter density and a sample of magnetic field lines, with the stellar magnetic field B_⋆ = 1 kG and the resistivity α_m = 1, in the cases with the stellar rotation rates Ω_⋆ = 0.1Ω_br (top panel) where a stable accretion column is formed (DC for disk+column) and Ω_⋆ = 0.15Ω_br (middle panel) in which the faster stellar rotation prevents the stable accretion column formation (D for disk only). The bottom panel shows the third case, with the stellar magnetic field B_⋆ = 0.5 kG, resistivity α_m = 0.1, and the rotation rate Ω_⋆ = 0.1Ω_br, in which a conical outflow is formed (DCE for disk+column+ejection).