Fluxes for the case with Ω_⋆ = 0.1Ω_br, B_⋆ = 0.5 kG, and α_m = 1. Left panel: mass flux across the disk at R = 12R_⋆ (solid line), onto the star (dotted line) and into the stellar wind (dashed line) in units of . Right panel: angular momentum flux of the matter in-falling onto the star from the distances below (solid line) and beyond (dashed line) the corotation radius and in the stellar wind (dotted line) in units of stellar angular momentum. Vertical solid lines mark the interval in time in which an average is taken to compute the quasi-stationary state.