Hydrodynamical simulations of planet rebound migration in photo-evaporating disks

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Table 2

Main parameters of the simulations.

Description	s = d log Σ₀ /d log r	Ṁ_PE [M_⊙ yr⁻¹]	h₀	Planet [resolution]^a	Rebound status^b
run-fid	−0.5	3.2 × 10⁻⁸	0.052	Neptune [M]	Yes
				Super-Earth [H]	Yes
				Saturn [M]	No
				Jupiter [L]	Yes
run-dl	−1	3.2 × 10⁻⁸	0.052	Neptune [M]	Yes
run-ph	−0.5	1.6 × 10⁻⁷	0.052	Neptune [M]	No
run-pl	−0.5	6.4 × 10⁻⁹	0.052	Neptune [M]	No
run-ah	−0.5	3.2 × 10⁻⁸	0.07	Neptune [M]	No
run-al	−0.5	3.2 × 10⁸	0.04	Neptune [M]	Yes

Notes. (a) L, M, and H stand for the low, medium and high grid resolutions (see the main text). (b) Yes and No correspond to the magnitude of rebound migration being larger or smaller than 3%, respectively.

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