Fig. 6

Changes of the outflow speed at the midplane of the disc according to the planetary mass. Each panel corresponds to each result obtained from different simulations at t = tend. Colour contour represents the flow speed in the radial direction. In order to show the differences of the outflow speed specifically, we plotted in a logarithmic scale. We note that the colour contour is saturated for the inflow (vr < 0) region. The orange-red and yellow areas mostly correspond to the regions where the radial velocity is positive or negative, respectively (see Fig. 2). The solid lines correspond to the specific streamlines of the gas flow. The black dashed line corresponds to the Bondi radius of the planet. The green dashed line shown in panels e and f corresponds to the Hill radius. We note that the length of the arrows does not scale with the flow speed.
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