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

Open Access

Fig. 3

Generated H₂O, ¹²CO₂ and ¹³CO₂ spectra for the models with no cavity (top row), a 1 AU cavity (middle row), and a 5 AU cavity (bottom row). The vertical colored bars indicate the integration ranges for the H₂O 15.17 and 17.22 µm flux (blue), as well as the ¹²CO₂ and ¹³CO₂ Q-branches (green and purple respectively).

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