Fig. 5.
Overabundance (mass fraction relative to solar; X/X⊙) of stable isotopes in the ejecta of simulation G14aNKK after decaying for 1016 s (0.32 Gyr). The striking production of 48Ca, 50Ti and 54Cr is a partcular hallmark of deflagrations in degenerate media high-density (see, e.g. Woosley 1997). The DDT simulation N100DDT from Seitenzahl et al. (2013a) is plotted for comparison, decayed to 2 Gyr.
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