中文

Hypernova Nucleosynthesis and Implications for Cosmic Chemical Evolution

天体物理学 2016-11-03 v1

摘要

We examine the characteristics of nucleosynthesis in 'hypernovae', i.e., supernovae with very large explosion energies (\gsim1052\gsim 10^{52} ergs). Implications for the cosmic chemical evolution and the abundances in M82 are discussed.

引用

@article{arxiv.astro-ph/0101469,
  title  = {Hypernova Nucleosynthesis and Implications for Cosmic Chemical Evolution},
  author = {Takayoshi Nakamura and Hideyuki Umeda and Koichi Iwamoto and Ken'ichi Nomoto and Masa-aki Hashimoto and W. Raphael Hix and Friedrich-Karl Thielemann},
  journal= {arXiv preprint arXiv:astro-ph/0101469},
  year   = {2016}
}

备注

To appear in 'Cosmic Evolution' Conference at IAP, Paris, honoring Jean Audouze and Jim Truran, 13-17 Nov 2000