Binary White Dwarf Supernova - V1 (Feb 2025)
Binary White Dwarf Supernova - V1 (Feb 2025)
Illustration of a star system consisting of two white dwarfs, in which one of the stars (right) is
transferring gas to its partner owing to their proximity. As a result, the star on the left has
reached an unstable, critical mass, which is resulting in a devastating explosion called a
supernova.
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