Molecular diagnostics for the mid-infrared emission of planet-forming disks - Carbon and oxygen elemental abundances

Open Access

Fig. D.1

Abundance and line emitting region (red line) of H₂O. The solid black lines indicate the gas temperatures of 300 K and 1000 K, the dotted line indicates the $τ_{H_{2} O} = 1$ $Mathematical equation: $\tau_{\mathrm{H}_{2} \mathrm{O}}=1$$ line. Each panel corresponds to the same model illustrated in Fig.1.

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