Fig. 14
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Mass fluxes generated from the photolysis of precursor gases in the upper atmosphere (p < 10 μbar) of K2-18 b. Reb, blue, and orange lines correspond to precursors of C, N, and S composition, respectively. The black dashed line sums contributions from C and N precursors and the black dotted line includes also the sulphur contribution. The results correspond to the nominal UV flux.
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