Simulations demonstrate that streaming instability and vertical shear instability driven by dust-gas interactions can produce characteristic shuttlecock dust substructures and dust-to-gas ratios of 20-50 in viscous protoplanetary disks.
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Substructures Induced by Dust Drag in Protoplanetary Disks
Simulations demonstrate that streaming instability and vertical shear instability driven by dust-gas interactions can produce characteristic shuttlecock dust substructures and dust-to-gas ratios of 20-50 in viscous protoplanetary disks.