Image Details
 
                    Caption: Figure 16.
Multi-epoch snapshots for the hydrodynamical simulation of a 1049 erg shock in the envelope of a ﹩6.93{{\rm{M}}}_{\odot }﹩ AGB star. We show the density (top row), temperature (middle row), and velocity (bottom row) vs. Lagrangian mass (left column) and radius (right column). In each panel, the solid line refers to the MESA results and the dashed line to the V1D results.
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