Towards a global model for planet formation in layered MHD wind-driven discs - A population synthesis approach to investigate the impact of low viscosity and accretion layer thickness

Open Access

Fig. 3

Migration rate as a function of orbital distance and planetary mass for the exemplary disc evolution at 3 Myrs (see Sect. 2.1.5). The cyan line marks the transition from type I to type II migration through gap opening. The pink line denotes the transition into the wind-driven type II migration regime. The left panel shows the migration map for Σ_active = 0.1 g/cm² and the right panel shows the migration map for Σ_active (0.08×c_s).

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