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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 4.

Dynamics of explosion models expressed by tracer particles for B12 ﹩\beta ﹩ 4.00 (left) and B11 ﹩\beta ﹩ 0.25 (right). The distribution of particles is shown in a quarter of each panel at the moment the jet-head reaches 1000, 2000, 3000, and 4000 km, respectively. Corresponding times after the bounce are shown in each panel: 10, 25, 52, and 100 ms for prompt-jets and 50, 66, 84, and 109 ms for delayed-jets, respectively. The color scale indicates ﹩{Y}_{{\rm{e}},\mathrm{nse}}﹩, ﹩{Y}_{{\rm{e}}}﹩ at the end of NSE.

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