Fig. 2

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Azimuthal profiles of various quantities at a fiducial radius of r = 60 au = 1.5 rp, and at an altitude of θ = 0.2 rad above the midplane in our Mp = 3 × 10−4M⊙ simulations. In the 3T case, azimuthal asymmetries of even a few percent in disk illumination that might be induced by the RWI, and are visible in the Td profile lead to strong nonaxisymmetry in ρ, Tg, and the velocity components.
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