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- W2009675261 abstract "Abstract Type Ia supernovae (SNe Ia) are very successfully used as standard candles on cosmological distance scales, but so far the nature of the progenitor(s) is unclear. A possible scenario for SNe Ia are merging carbon/oxygen white dwarfs with a combined mass exceeding the Chandrasekhar mass. We determine the theoretical rates and delay time distribution of these mergers for two different common envelope prescriptions and metallicities. The shape of the delay time distributions is rather insensitive to the assumptions. The normalization is a factor ~3–13 too low compared to observations." @default.
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- W2009675261 date "2011-07-01" @default.
- W2009675261 modified "2023-09-26" @default.
- W2009675261 title "Double White Dwarf Merger Rates" @default.
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- W2009675261 doi "https://doi.org/10.1017/s1743921312015086" @default.
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