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

Open Access

Fig. 5

Synthetic H₂O spectra of the fiducial model using the chemical network (black) and three models with parameterized abundances (blue, pink, and red) between 23.7 and 24 μm. The flux is normalized to the 9_8,1−8_7,2 line at 23.87 μm.

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