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Effect of lift force on the aerodynamics of dust grains in the protoplanetary disk

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Figure

Figure 1 rd dependence of tcol (solid lines) and tspin-down (dashed lines) at R1 = 1. tcol is always longer than tspin-down in the Stokes regime.
Figure 2 Parameter space where the dust grains can keep spinning in thelines. The condition R1–rd plane
Figure 3 Dependence of the grain velocity on the direction of the spin angular momentum.x We show the grain velocity in the radial direction (the solid line) and in the azimuthal direction y (the dashed line)
Figure 2 moves down and that the blue region expandsinside. When fd is approximately 0.1, the blue regionincludes the dotted magenta line, which shows the grain
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