Fig. 7

Surface density perturbation (Σ − Σ0(r))∕Σ0(r) relative to the equilibrium state before planet insertion. The figure is taken at t = 3500 Porb and shows the reference non-radiative simulation (top) and the simulation with stellar irradiation (bottom) for the fiducial set of parameters. The outer gap edge in the bottom panel exhibits additional azimuthal asymmetries.
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