Migration of Jupiter mass planets in discs with laminar accretion flows

Open Access

Table 1

Simulations names and main parameters.

Name	Σ_A (g cm⁻²)	Ṁ_A(M_⊙ yr⁻¹)	Ṁ_D(M_⊙ yr⁻¹)
NW	0	0	− 8 × 10⁻¹¹
S01	0.1	− 10⁻⁸	− 8 × 10⁻¹¹
S1	1	− 10⁻⁸	− 8 × 10⁻¹¹
S10	10	− 10⁻⁸	− 8 × 10⁻¹¹
H_in	110	− 10⁻⁸	− 8 × 10⁻¹¹
H_out	110	10⁻⁸	− 8 × 10⁻¹¹

Notes. The accretion flow transported by the disc’s active layer is labelled Ṁ_A, while Ṁ_D is the stellar accretion rate due to viscosity. The minus sign indicates inflow. Notice the in the control simulation Hout we apply a radial outflow in the vicinity of the disc midplane.

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