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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 5.

Disk evolution time series seen at λ = 1.25 mm dust emission, convolved with the same beam as Figure 4. Dust is initiated with a constant dust-to-gas ratio. Over time VSI turbulence shuts down, which results in a razor-thin disk of large grains.

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