Mid-infrared spectra of T Tauri disks: Modeling the effects of a small inner cavity on CO2 and H2O emission

Open Access

Fig. 12

Gas temperature in a vertical cut at 0.3 AU, plotted as a function of CO₂ (solid lines) and H₂O (dashed lines) column density. This is shown for the full disk models with f_ℓ = 0.9 (blue), 0.99 (green), and 0.999 (black; the fiducial model).

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