Fig. 3
Abundances after 7 Myr evolution for four different model setups. Panel a: inheritance scenario with low ionisation and evolving disk structure. Panel b: reset scenario, high ionisation and evolving disk structure. Panel c: inheritance scenario with high ionisation and static (unchanging) disk structure. Panel d: inheritance scenario with high ionisation and evolving disk structure. The blue, red-and-black and green arrows to the right of each panel indicate the initial abundances assumed for H2O, CO/CO2 and CH4, respectively, in the inheritance scenario.
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