Fig. 10

Dependence of the normalized torque γΓ∕Γ0 on the planet mass Mp (top) and α viscosity (bottom). Additionally, the top horizontal axis of each panel shows the position of the outer gap edge redge as resulting from Eq. (24). Circles and solid black lines correspond to simulations with gap irradiation; diamonds and dashed grey lines correspond to reference non-radiative simulations. Open symbols correspond to simulations without torque oscillations (i.e. Rossby-stable) while filled symbols mark simulations with gap edge instabilities. Data points are labelled with the corresponding torque reduction factor firr (Eq. (35)). Clearly, gap edge irradiation reduces the magnitude of the torque (or even causes torque reversal) for Mp < 1 MJ and α > 10−3.
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