A white dwarf undergoes carbon detonation only if it has a normal binary star companion close enough for the dwarf star to siphon sufficient amounts of matter onto itself, the siphoned matter having been expelled during the process of the companion's own late stage stellar evolution.
The siphoned matter having been expelled during the process of the companion's own late stage stellar evolution. A white dwarf undergoes carbon detonation only if it has a normal binary star companion close enough for the dwarf star to siphon sufficient amounts of matter onto itself.
A white dwarf undergoes carbon detonation only if it has a normal binary star companion close enough for the dwarf star to siphon sufficient amounts of matter onto itself. The siphoned matter having been expelled during the process of the companion's own late stage stellar evolution.
A white dwarf undergoes carbon detonation only if it has a normal binary star companion close enough for the dwarf star to siphon sufficient amounts of matter onto itself. The siphoned matter having been expelled during the process of the companion's own late stage stellar evolution.