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Cited article:

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A Fast Second-order Solver for Stiff Multifluid Dust and Gas Hydrodynamics

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The Dependence of the Structure of Planet-opened Gaps in Protoplanetary Disks on Radiative Cooling

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Dust Coagulation Reconciles Protoplanetary Disk Observations with the Vertical Shear Instability. I. Dust Coagulation and the VSI Dead Zone

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