Figure 24 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 24.

Radial distribution of heating rates for 1D model at t _pb = 150 (red lines), 250 (green lines), and 350 ms (blue lines). LB models (thin lines) tend to overestimate the heating rate in a pre-shock region and underestimate in a post-shock region.

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