Polydisperse formation of planetesimals - The dust size distribution in clumps

Open Access

Fig. 10

Normalised mean size distribution at the 99^th percentile and between 135 ≤ Ωt ≤ 145 using the same PSI runs and colour scheme as Figure 9. The dashed line indicates the Stokes number at resonance velocity $v_{d}_{x}^{0} (τ_{s}) = {\bar{u}}_{x}^{0} (σ)$ $v_{\mathrm{d}}{}_{x}^{0}\left(\tau_{\mathrm{s}}\right)=\bar{u}_{x}^{0}(\sigma)$ , and the dot-dashed line shows the average Stokes number at Ωt = 0.

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