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Azimuthal Dust Polarization from Aerodynamically Aligned Grains as Evidence for the Streaming Instability in Protoplanetary Disks

  • Authors: Zhe-Yu Daniel Lin, 哲宇 林, Jeonghoon Lim, 정훈 임, Jacob B. Simon, Zhi-Yun Li, Daniel Carrera, Manuel Fernández-López, Rachel Harrison, Rixin Li, 日新 李, Leslie W. Looney, Ian W. Stephens, Haifeng Yang

Zhe-Yu Daniel Lin et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure 4.

The polarization angle χ using Stokes Q and U summed over the spatial domain for each simulation taken at the last snapshot. The colors correspond to different levels of χ, where χ = 0° is polarization in the radial direction, while χ = ±90° is polarization in the azimuthal direction. Each simulation is initialized with a different combination of (τsZ). The circles denote cases with strong clumping, while the crosses denote cases without strong clumping. The squares highlight the two examples explored in more detail in Figures 1, 2, and 3.

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