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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 5.

Dust–gas density ratios, ρd/ρg, at the final snapshots for different models. The model names and the corresponding maximum dust–gas density ratios within the radial range R ∈ [3, 10] are indicated in the top-right corner of each panel.

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