The colour contour shows the difference of flow speed from the Keplerian shear obtained by m05 run at t = t_end. We plotted |v − v_∞(x)|∕|v_∞(x)|, where v is the gas velocity and v_∞(x) is the Keplerian shear expressed by Eq. (10). The contour shows that the spherical region around the planet is highly influenced by the gravity. We note that the red region along x = 0 is not the outflow but the horseshoe flow. We also note that the colour contour is saturated in the region coloured with red. The grey solid lines correspond to the specific gas streamlines. We highlighted the atmospheric recycling streamline in the thick white solid line. The red, orange, green, blue, and purple dashed lines are the circles of radius R_Bondi, 1.5 R_Bondi, 1 [H], 2 [H], and 3 [H].