Figure 11 from Self-consistent Ring Model in Protoplanetary Disks: Temperature Dips and Substructure Formation

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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 11.

The effects of density floor on temperature profiles for one population. The dust peak surface density is 0.2 g cm⁻². From top to bottom, the density floors are 0.1, 0.01, 0.001, and 0001. The temperature dip becomes stronger with a lower-density floor.

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