Figure 1 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 1.

Pre-collapse composition distributions for the 15 M _☉ stars of Limongi & Chieffi (2006; LC15, top left), Woosley & Weaver (1995; WW15, bottom left), and Woosley et al. (2002; WHW15, top right), and for the 11.2 M _☉ star of Woosley et al. (2002; WHW11, bottom right).

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