Fig. 3
Upper panel: torque exerted on a 3 M⊕ planet as a function of its orbital distance. The solid line corresponds to the analytical prescription of Paardekooper et al. (2011). Triangles and diamonds are the results from hydrodynamical simulations with/without the effects due to the waves generated by the other planets included. Lower panel: same but for mp = 6 M⊕.
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