Time-resolved protoplanetary disk physics in DQ Tau with JWST

Open Access

Fig. 9

Upper panel: Rovibrational H₂O lines in the spectra of DQ Tau. Middle panel: Rotational H₂O (solid marks) and OH (dotted marks) lines in the spectra of DQ Tau. Lower panel: rotational H₂O lines (solid marks) with their upper level energies in K indicated above the panel.

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.