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Fig. 4

image

Aspect ratio as a function of the orbital distance for discs with a viscosity of α = 5 × 10−3. Left: aspect ratio for discs with different water abundances that feature a transition in the dust fragmentation velocity from 1 to 5 m s−1 and a dust-to-gas ratio of 1%. Right: aspect ratio of discs with different dust-to-gas ratios that feature a transition in the dust fragmentation velocity from 1 to 5 m s−1. Furthermore, we show the effects of a transition in the fragmentation velocity from 1 to 10 m s−1 for a disc with a dust-to-gas ratio of 1%.

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