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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 B1.

Slices through our three-dimensional dust opacity tables for the Planck opacities (function of ﹩{a}_{{\rm{\max }}}﹩, q, and T), used in all hydrodynamic simulations.

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