Figure 20 from Revisiting Impacts of Nuclear Burning for Reviving Weak Shocks in Neutrino-driven Supernovae

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Revisiting Impacts of Nuclear Burning for Reviving Weak Shocks in Neutrino-driven Supernovae

Authors: Ko Nakamura, Tomoya Takiwaki, Kei Kotake, and Nobuya Nishimura

Nakamura et al. 2014 The Astrophysical Journal 782 91.

Provider: AAS Journals

Caption: Figure 20.

Time evolution of chemical compositions of flow A, B, and C. The results from the pseudo-flashing method (top panels) and network calculation (bottom) are shown.

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