Average azimuthal velocity v_ϕ profile of the outer disk for run 1 (purple solid line) and run 2 (solid), run 3 (dashed), run 4 (dotted), run 5 (solid) at t = 50 kyr (left panel), t = 100 kyr (middle panel), and t = 150 kyr (right panel). The darker the color of a line, the larger the inclination angle α. We note that v_ϕ was computed within a vertical extent of |z| < max(6 AU, 0.05r) from the midplane of the disk for 300 logarithmically spaced radial bins in the range from 10 to 10⁴ AU. The gray line is the Keplerian profile for a 2.5 M_⊙ star.