MIRACLE - I. Unveiling the multi-phase, multi-scale physical properties of the active galaxy NGC 424 with MIRI, MUSE, and ALMA

Open Access

Fig. C.1.

Comparison of the observed (top panel) and best-fit MOKA^3D (middle panel) moment maps for the H₂S(1) emission line. Residuals are shown in the bottom panel. The modelling and best-fit parameters are presented in Sect. 4.1 and listed in Tab. 2. North is up, east to the left.

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.