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Planetesimal Formation under Realistic Gas Dynamics: Dust Concentration in Turbulent and Windy Protoplanetary Disks

  • Authors: Pinghui Huang, Xue-Ning Bai

Pinghui Huang and Xue-Ning Bai 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure 4.

The CDFs of the dust–gas density ratio, computed by counting the number of grid cells, ﹩P[({\rho }_{{\rm{d}}}/{\rho }_{{\rm{g}}})\gt {({\rho }_{{\rm{d}}}/{\rho }_{{\rm{g}}})}_{{\rm{threshold}}}]﹩. The CDFs are calculated using data from the last 500 innermost orbits (1500P0–2000P0 for all models except “S2”, for which 1700P0–2200P0 is used). The solid lines and shaped regions are the temporal averages and standard deviations. The calculation of the CDFs covers R ∈ [3, 10] and ﹩z\in [-{z}_{{\rm{tr}}},\,{z}_{{\rm{tr}}}]﹩. For the CDF calculation across different refinement levels, cells on coarser levels are converted into an equivalent number of finest-level cells before performing the statistics.

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