Failure to Detonate (IMAGE)
Caption
A collaboration led by George Jordan at the University of Chicago's Flash Center for Computational Science has conclusively demonstrated a connection between white dwarf stars that fail to completely detonate and a class of oddly dim supernovae. This image, based on supercomputer simulations, shows the asymmetric surface characteristics of a white dwarf that fails to detonate.
Credit
Courtesy of Brad Gallagher, George Jordan/Flash Center for Computational Science
Usage Restrictions
News organizations may use this image in connection with reports on the University of Chicago's Flash Center for Computational Science.
License
Licensed content