- #1
bbbl67
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Okay, so for years the typical mechanism used to describe a white dwarf supernova explosion was that a white dwarf accumulates matter from a main sequence binary companion. Then a few years later, the concept of two white dwarfs crashing into each other came up. With the main sequence companion, at least you could see how the mass would stop accumulating at 1.4 solar masses (the Chandrasekhar Limit). But with two white dwarfs, don't both white dwarfs completely obliterate each other? What if the combined mass of the two white dwarfs was above 1.4 solar masses? How can you call the resultant Type Ia supernova the same as any other Type 1a? Wouldn't it be a far bigger explosion?