Fig. A.1
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Schematic of the expected meridional velocity (υθ) from a VSI-unstable disk with an embedded massive planet. Top: Face-on view, red (blue) indicates gas moving toward (away from) the disk midplane. Bottom: Edge-on view (radius vs. height) of the azimuthally averaged prediction, red (blue) indicates gas moving downward (upward); gray indicates the gas density.
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