Fig. 16

Torques exerted on the planet in models 4/4+ (upper panel) and 5/5+ (lower panel). Significant departures can be observed only for the outer disk torque (Γouter disk), which eventually explains the decline of the total torque, Γtot, (see orange solid and dashed curves for models 4/5 and 4+/5+, respectively) in the models where stellar motion is taken into account.
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