Fig. 13
Integrated line fluxes from TW Hya models (Mdisk = 2.3 × 10-2M⊙, ψ = 0.3 and hc = 0.1) with different amounts of carbon depletion (hexagons; left side) and oxygen depletion (right side). The black bars show the observations for TW Hya (Schwarz et al. 2016; Kama et al. 2016b, and references therein). The purple crosses show the results from Kama et al. (2016b), recalculated for δC = δO = 0.01, [D]/[H] = 2 × 10-5 (cf. Sect. 4.4).
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