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Rapid Dust Growth during Hydrodynamic Clumping due to Streaming Instability

Rapid Dust Growth during Hydrodynamic Clumping due to Streaming Instability

Abstract Streaming instability is considered to be one of the dominant processes in promoting planetesimal formation by the gravitational collapse of dust clumps. The development of streaming instability is expected to form dust clumps in which the local dust density is strongly enhanced and even greater than the Roche density. …