Hypernova Nucleosynthesis and Implications for Cosmic Chemical Evolution
arXiv:astro-ph/0101469 · doi:10.1142/9789812810830_0039
Abstract
We examine the characteristics of nucleosynthesis in 'hypernovae', i.e., supernovae with very large explosion energies ($\gsim 10^{52}$ ergs). Implications for the cosmic chemical evolution and the abundances in M82 are discussed.
To appear in 'Cosmic Evolution' Conference at IAP, Paris, honoring Jean Audouze and Jim Truran, 13-17 Nov 2000