Figure 9 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 9.

Maximum density and temperature of ejecta with ﹩{Y}_{{\rm{e}}}﹩ for a prompt model, B11 ﹩\beta ﹩ 1.00 (upper), and a delayed model, B11 ﹩\beta ﹩ 0.25 (lower). The ﹩{Y}_{{\rm{e}},\mathrm{nse}}﹩ of each particle is shown in the given color range.

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