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Fig. 17

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Time evolution of an unstable dust ring in a 3D simulation with parameters τ0 = 4 × 10−3, Z = 0.03, and A = 0.4. The dashed and solid curves are the initial and current mid-plane gas pressure profile, respectively. One can clearly see an amplification of the gas pressure bump and unstable behavior of the dust ring, as it develops strong non-axisymmetries and splits ofa vortex which subsequently migrates inward.

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