Theoretical 3D diagrams of the MUSE IFU data for NGC 3081. The panel layout and model grid parameters are the same as in Figure 1, except that the fast-shock model adopts ﹩{\sigma }_{[{\rm{O}}{\rm{III}}]}=\frac{2}{3}{v}_{s}﹩, following M. G. Allen et al. (2008) to account for thermally unstable shocks, whose behavior resembles that of steady-flow shocks with velocities of ﹩\sim \frac{2}{3}{v}_{s}﹩. The interactive version of this figure allows the reader to zoom and rotate any of the four panels. Hovering the mouse over a point displays the object name and its x, y, and z coordinates. In addition, the standard Plotly toolbar commands are available, including the option to reset the view to the default orientation.

An interactive version of this figure is available in the online article.

An interactive version of this figure is available.

An interactive version of this figure is available in the online journal.