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Fig. 2

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Abundance maps of H2O (left column) and CO2 (middle column) for the models with no cavity (top row), a 1 AU cavity (middle row) and a 5 AU cavity (bottom row). 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 right column shows the gas temperature, with dashed black lines indicating 100 and 300 K. The yellow contours indicate the region in which 90% of the H2O 113,9 − 100,1o line emission at 17.22 µm (Eup = 2438 K) originates. The red contours indicate the origin of 90% of the CO2 v2 = 1 − 0 Q(20) line emission (Eup = 1196 K).

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