Fig. A.1
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θ-component of vorticity at θ = 0.2, with respect to the initial condition, in units of the planet’s orbital frequency Ωp. Between 200 and 250 orbits, the vorticity profile is largely unchanged in the β-cooling simulations, but deviates strongly in the 3T case as radiation couples to the asymmetries generated by disk-planet interaction.
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