Figure 6 from

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF

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

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

Caption: Figure 6.

Space−time (R−t) plot for the maxima of dust–gas ratios ﹩{\rm{\max }}{({\rho }_{{\rm{d}}}/{\rho }_{{\rm{g}}})}_{z}﹩ for different models.