Fig. 8
Settling fraction fset as function of planet mass for αz = 10−2, hgas = 0.05, η = 5 × 10−3, τs = 0.1 and M⋆ = 1 M⊙. Turbulence is assumed to be isotropic and the correlation time tcorr = Ω−1. Curves give fset when it is calculated based on the laminar-only velocity (dashed), turbulent rms velocity (gray), and for a distribution of velocities (solid).
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