Speaker
Prof.
Ken Nomoto
(IPMU, University of Tokyo)
Description
The properties of supernovae associated with GRBs & XRFs, and some other
related supernovae are summarized. Discussion includes the possible
connection to the unusual supernovae, such as extremely luminous and
extremely faint supernovae. The abundance patterns predicted in their
nucleosynthesis are compared with those of metal-poor halo stars, DLAs, and
other related objects.
Primary author
Prof.
Ken Nomoto
(IPMU, University of Tokyo)
