Fig. 7
Final temperature profile of irradiated (dashed grey lines) and non-irradiated (black lines) discs for two particular simulations (Σ0 = 95.844 g cm-2, acore = 46, γ = 0.9; and Σ0 = 502.52 g cm-2, acore = 80, γ = 0.9) as a function of the distance to the star. Coloured dots represent the ice line positions of H2O, CH3OH, NH3, CO2, H2S, CH4, CO, and N2. Models without clathrates.
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