Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 2.

The gas density normalized by the initial density profile in the midplane, ρg/ρg,init,midplane at the final snapshots for different models (taken at t = 2000P0 for all models except “S2,” which is shown at t = 2200P0). The contours indicate the poloidal magnetic flux.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse