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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 4.

RADMC-3D models of our simulation data at 1.25 mm dust continuum (red color maps; rows one and two), and 1.6 µm wavelength, showing scattered light (blue color maps; rows three and four). Dust continuum images have been convolved with a beam identical to the observations published in M. Villenave et al. (2022); scattered light images have been convolved with a circular Gaussian beam with a 30 mas FWHM. The innermost 1 au of the images has been masked before the beam convolution.

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