Simulations show that dust in gravitationally fragmenting protoplanetary disks grows to decimeter sizes and concentrates into dense clump centers, which may seed giant planet formation.
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Gravitoviscous protoplanetary disks with a dust component. II. Spatial distribution and growth of dust in a clumpy disk
Simulations show that dust in gravitationally fragmenting protoplanetary disks grows to decimeter sizes and concentrates into dense clump centers, which may seed giant planet formation.