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Fig. A.1

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Abundance maps of H2O (first and second columns) and CO2 (third and fourth columns) for the models with no cavity (top row), a 1 AU cavity (middle row), and a 5 AU cavity (bottom row) for the fiducial grid without H2O ro-vibrational cooling (first and third columns) and the grid with H2O ro-vibrational cooling (second and fourth columns). The H2O and CO2 snowlines (defined as ngas/nice = 1) are indicated with solid light blue and pink lines, respectively. The dashed, dark blue line shows the dust τ = 1 surface at 15 µm. The yellow contours indicate the region in which 90% of the H2O 113,9 − 100,10 line emission at 17.22 µm (Eup = 2438 K) originates. The red contours indicate the origin of 90% of the CO2 0110 − 0000 Q(20) line emission (Eup = 1196 K).

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