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pro vyhledávání: '"Shilun Jin"'
Autor:
Shilun Jin, Noam Soker
Publikováno v:
The Astrophysical Journal, Vol 971, Iss 2, p 189 (2024)
The common envelop jet supernovae (CEJSNe) r -process scenario has been proposed as an r -process nucleosynthesis site in the past decade. Jets launched by a neutron star that spirals in inside the core of a red supergiant star in a common envelope e
Externí odkaz:
https://doaj.org/article/0597ac14a8ba484d82560b194498a4e5
Autor:
Ziming Li, Jie Zhu, Taofeng Wang, Minliang Liu, Jiansong Wang, Yanyun Yang, Chengjian Lin, Junbing Ma, Peng Ma, Zhen Bai, Yuechao Yu, Xing Zhang, Xingquan Liu, Fangfang Duan, Chengui Lu, Herun Yang, Xianglun Wei, Junwei Zhang, Shilun Jin, Zhihao Gao, Yue Hu, Yongjin Yao, Jianguo Wang, Song Guo, Wei Jiang, Biao Yang, Jianjun He
Publikováno v:
Physical Review C. 107
Autor:
Shilun Jin
Publikováno v:
The Astrophysical Journal. 927:116
The weak r-process offers an explanation of the formation of lighter heavy elements 36 ≤ Z ≤ 47 in ultra-metal-poor stars. Magnetohydrodynamically driven supernovae are thought to be a robust astronomical site of the weak r-process and recently g
Publikováno v:
Nature. 588(7836)
The rate of the triple-α reaction that forms