Fig. 18
Accretion probability as a function of the planetary mass and the Stokes number for the Mach number
and 0.1 (bottom to top) in the UP case (left column), the PI-Stokes case (middle column), and the PI-Epstein case (right column). The contours represent the accretion probabilities. We assume α = 10−3. The gray-shaded region is the region where Pacc = 0.
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