Understanding JWST water spectra: What can thermochemical models tell us about the (cold) water in protoplanetary disks?

Open Access

Fig. A.8

Maps of the H₂ density, UV radiation field G₀, and gas temperature of the fiducial chemistry model. The solid black (and white in the second panel) contours represent the H₂O abundance structure of the fiducial parameterized model (see Fig. 1).

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