Image Details

Choose export citation 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 4.

Top: The dust opacities used for the disk with a single-dust population. Optical constants are from DSHARP (Birnstiel et al. 2018). The minimum grain size is 0.1 μm. At short wavelengths, the opacity decreases as the ﹩{a}_{\max }﹩ increases. Blue, orange, green, red, and purple denote ﹩{a}_{\max }﹩ = 1 μm, 10 μm, 100 μm, 1 mm, and 1 cm cases, respectively. Solid curves represent absorption opacities (﹩{\kappa }_{\nu }^{\mathrm{abs},\mathrm{tot}}﹩), and dashed curves represent scattering opacities (﹩{\kappa }_{\nu }^{\mathrm{sca},\mathrm{tot}}﹩). Bottom: The opacities used for disks with two dust populations. The opacities between 0.1 mm and 1 cm are marked in red-brown.

Other Images in This Article
Copyright and Terms & Conditions