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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 3.

Top panels: the x-axis profile of the midplane ϵ averaged along the y-axis plotted against time (the horizontal axis). The contours show 〈ϵy = [1, 3, 10]. Middle panels: the x-axis profile of Stokes 〈Iy, which is Stokes I averaged along the y-axis. Bottom panels: the corresponding χ also from Stokes Q and U averaged along the y-axis. The left and right columns correspond to the two simulations with (τsZ) = (0.01, 0.03) and (0.03, 0.005), respectively. Note that the x-axis has a shear-periodic boundary condition.

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