TIL about accretion-induced collapse of white dwarfs, aka "not all white dwarfs that reach the Chandrasekhar mass limit go supernovae" https://iopscience.iop.org/article/10.1086/307119/fulltext/ …
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models suggest that under the right conditions, carbon flares will occur but not large enough to actually cause mass loss, allowing the WD to burn accreted helium while continuing to grow https://arxiv.org/pdf/1706.03843.pdf …
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they're apparently a very interesting possible NS creation pathway, with possible implications for pulsar populations (ex: millisecond pulsar formation). https://sci-hub.tw/10.1111/j.1365-2966.2009.15988.x …
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