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Fig. 7

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Specific radial torque density in units of (dΓ/dm)0 (see Eq. (36)) for embedded planet models using the ϵ potential with various ϵp. The simulations use a given H = 0.05, and the x-axis refers to the radial coordinate where ap is the semi-major axis of the planet. The planet to star mass-ratio is q = 6 × 10-5. Other parameters of the simulations are stated in Sect. 4.3.

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