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Fig. 7

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H2O abundance maps of four models using the chemical network with varying accretion luminosity. The τ = 1 surface of the dust continuum at 15 μm is indicated with a dashed blue line. Red, pink, and blue contours represent the 70% emitting regions of the H2O 177,10−164,13 (Eup = 6371K), 113,9−100,10 (Eup = 2438K), and 83,6−70,7 (Eup = 1447K) lines, respectively.

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