Figure 2 from THE r-PROCESS NUCLEOSYNTHESIS IN THE VARIOUS JET-LIKE EXPLOSIONS OF MAGNETOROTATIONAL CORE-COLLAPSE SUPERNOVAE

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THE r-PROCESS NUCLEOSYNTHESIS IN THE VARIOUS JET-LIKE EXPLOSIONS OF MAGNETOROTATIONAL CORE-COLLAPSE SUPERNOVAE

Authors: Nobuya Nishimura, Tomoya Takiwaki, and Friedrich-Kerl Thielemann

2015 The Astrophysical Journal 810 109.

Provider: AAS Journals

Caption: Figure 2.

Abundances of heavy elements at NSE. The total mass fraction of heavy nuclei (X_A), defined by their atomic mass, ﹩A\geqslant 6﹩, are plotted in a typical density range. The cases of ﹩{Y}_{{\rm{e}}}=0.05﹩, 0.10, 0.15, and 0.20 are calculated with a constant temperature T = 9 GK.

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