A volume rendering of the density after the merger of a 0.6 and 0.9 solar mass white dwarf. This image is from a calculation that was performed on ORNL's Titan supercomputer. The infrastructure for modeling white dwarf mergers with Castro is provided in the wdmerger git repo.
- White Dwarf Mergers on Adaptive Meshes. I. Methodology and Code Verification, M. P. Katz, M. Zingale, A. C. Calder, F. D. Swesty, A. S. Almgren, & W. Zhang, 2016, ApJ, 819, 94