Figure 2 from Self-consistent Ring Model in Protoplanetary Disks: Temperature Dips and Substructure Formation

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Self-consistent Ring Model in Protoplanetary Disks: Temperature Dips and Substructure Formation

Authors: Shangjia Zhang, Xiao Hu, Zhaohuan Zhu, and Jaehan Bae

2021 The Astrophysical Journal 923 70.

Provider: AAS Journals

Caption: Figure 2.

The equilibrium temperature ratio between the single-sized big species and the small species calculated using DSHARP opacity. The stellar temperature is 6000 K. From left to right, the disk temperatures T_d are 20, 50, and 100 K.

Other Images in This Article

Copyright and Terms & Conditions