Fig. 3.
Time-integrated Rayleigh–Taylor growth factors vs. enclosed mass for the 1D hydrodynamic models B15, W16, W18, W18r, W18x, W20, and N20 at the given times. The vertical red and blue lines denote the mass coordinates of the (C+O)/He and He/H composition interfaces, respectively. These interfaces are Rayleigh–Taylor unstable after the passage of the SN shock.
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