CO2-rich protoplanetary discs as a probe of dust radial drift and trapping

Open Access

Fig. 5

Evolution of the vapour mass of H₂O (blue), CO₂ (bright green), and CH₄ (olive green) normalised to their initial values for a smooth disc in Scenario 1. The vertical dotted lines mark the times that each molecule reaches its peak vapour mass and the rightward arrows indicate the timescale for the peak to then decrease (Eq. (19)).

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