Dust ring and gap formation by gas flow induced by low-mass planets embedded in protoplanetary disks - I. Steady-state model

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Fig. 10

Dust surface density with m = 0.03 for the different Stokes numbers, the Mach numbers, and the turbulent parameters. Different colors correspond to different Stokes numbers. The minimum and the maximum values of the dust surface density are summarized in Figs. 13 and 14.

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