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

Open Access

Fig. A.9

H₂O abundance as a function of gas temperature and UV radiation field, following a simple chemical model (see Sect. A.4). The red and blue boxes represent the conditions within the inner and outer H₂O reservoir.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.