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Fig. 5


Vertical distribution of the abundances of selected molecules as calculated through each of the 16 models in which the space of metallicity, temperature, eddy diffusion coefficient, and stellar UV flux are explored. Each colour corresponds to a set of metallicity and temperature values and each line style to a set of eddy diffusion coefficients and stellar UV fluxes (see legend in the H2O panel and meaning of each symbol in Table 2).

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