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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 A1.

The top-left panel shows the poloidal gas velocity normalized by the sound speed, similar to Figure 1. The top-right panel shows the normalized gas density together with the magnetic flux, similar to Figure 2. The bottom panels present the dust–gas density ratios for two dust species (St1 = 0.1 and St2 = 0.01), similar to Figure 5. The maximum dust–gas ratios for the two species are indicated in the top-right corners of the corresponding panels.

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