Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

Just a Phase? Weakening Vertical Shear Instability Explains Class II Disk Morphologies: Simulations with Dust Coagulation, Sedimentation, Thermal Relaxation, and Backreaction

  • Authors: Thomas Pfeil, Alexandros Ziampras, Shangjia Zhang, 尚嘉 张, Philip J. Armitage, Yan-Fei Jiang, 燕飞 姜

Thomas Pfeil et al 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure D2.

Same as Figure 2 but for the four additional simulations. Columns (a) and (b) are the same simulation setup as columns (b) and (c) in Figure 2 and but with vfrag = 400 cm s−1. Columns (c) and (d) show simulations with different temperature stratification: in column (c), the transition height has been reduced to 3.8H; in column (d) it has been lowered to 3H.

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
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse