T Coronae Borealis Explosive Delay
This is a news story, published by Guardian, that relates primarily to the white dwarf’s news.
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brightest starGuardian
•Starwatch: Still waiting for nova T Coronae Borealis to blow up
71% Informative
T Coronae Borealis is a recurrent nova - it consists of two stars: a red giant and a white dwarf.
The white dwarf is a dense stellar core about the size of the Earth , whose gravity is stripping gas from the red giant.
Gas accumulates on the white dwarf’s surface before detonating in a thermonuclear explosion, causing the star to temporarily brighten.
This does not destroy the white dwarfed star, which then returns to normal and the cycle repeats.
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