Fig. 6
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Surface density deviations and vertical velocity maps at the mid-plane for our disk with an embedded subthermal-mass planet (h = 0.1, Mp = 0.3 Mth) at R = R0 after 500 planetary orbits. While the planet’s primary spiral is prominent in this color range, the VSI continues to operate as shown by the quasi-axisymmetric stripes of vertical motion in the bottom panel.
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