Trajectories of pebbles in Shear case (top) and PI-Stokes case (bottom) with different Stokes numbers at midplane around an embedded planet with m = 0.1. We set z_s = 0 for all cases. The red and blue solid lines correspond to the trajectories of pebbles which accreted and did not accrete onto the planet, respectively. The dashed and dotted circles show the Hill and the Bondi radius of the planet, respectively. The black dots at the center of each panel denote the position of the planet. The interval of pebbles at their initial locations is 0.05 [H].