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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 10.

Dust surface density of the big-grain population (top panels) and midplane temperature (bottom panels). (a) Model with α = 2 × 10−3, Σg = 4.1 g cm−2, ϵ = 0.01 at the ring. (b), (c) Models with α = 7 × 10−4 and with different radial resolutions. In these models small grains’ surface density is 100 × higher than that in model (a). The small grains’ densities are marked by gray solid curves and gas surface densities are marked by gray dashed curves.

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