Fig. A.2

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Velocity radial profiles for the VSI-unstable disk simulations without a planet (first column), with an embedded Saturn-mass planet (second column), and with an embedded Jupiter-mass planet (third column). The values displayed correspond to 3 pressure scale heights from the disk midplane for both disk hemispheres, shown by the blue dashed and orange solid lines. The radial location of the planets is indicated with a vertical black solid line.
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