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Fig. 2

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First 1 Myr evolution of a and e, and the absolute values of ta, te and ti for an inner planet (left panels) initially located at a = 0.016 au with e = 0.1 and an outer planet (right panels) initially located at a = 0.1 au and e = 0.5. The planet masses are MP = MMars. Solid lines indicate the results following the prescriptions from IDA20, and dotted lines show the corresponding results from CN08. The vertical lines indicate the moment at which e = hg, which separates the subsonic (e < hg) and the supersonic (e > hg) regimes.

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