Disc and atmosphere composition of multi-planet systems

Open Access

Fig. B.2

Disc accretion rate $\dot{M}$ $\[\dot{M}\]$ of water gas at 0.5 AU (solid lines) and water solids at 3.0 AU (dashed lines) over time of the unperturbed disc. Different colours represent the different viscosities (setups: V1noP, V5noP & V10noP). The water ice line is between 1 and 2 AU depending on the viscosity. Positive values indicate inward movement.

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