Fig. 8
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Ejecta properties for our RSG star explosion model as computed by HERACLES++ (solid) and V1D (dashed). For representative epochs between 2.8 h and 1.6 d, we show the density (top row), the temperature (middle row), and the velocity (bottom row) vs. the Lagrangian mass (left column) and radius (right column). (See Sect. 5.3 for discussion).
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