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Fig. 8

image

Trajectories of pebbles in UP-m003-hw01 case (left panel) and PI-Stokes-m003-hw01 case (right panel) with St = 10−4 at the midplane of the disk. We set zs = 0. The red and blue solid lines correspond to the trajectories of pebbles which accreted and did not accrete onto the planet, respectively. The dotted-dashed and dashed circles show the Bondi and the Hill radius of the planet, respectively. The sizes of the Bondi radius and the Hill radius are 0.03 [H] and 0.22 [H]. The black dots at the center of each panel denote the position of the planet. The interval of pebbles at their initial locations is 0.003 [H].

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