Failure to Detonate (IMAGE) University of Chicago 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 Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.