Late‐Time Convection in the Collapse of a 23<i>M</i><sub>⊙</sub>Star
Late‐Time Convection in the Collapse of a 23<i>M</i><sub>⊙</sub>Star
The results of a 3-dimensional SNSPH simulation of the core collapse of a 23 solar mass star are presented. This simulation did not launch an explosion until over 600ms after collapse, allowing an ideal opportunity to study the evolution and structure of the convection below the accretion shock to late …