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- W1691799114 abstract "We describe our first attempt at modelling nucleosynthesis in massive AGB stars which have undergone core carbon burning, the super-AGB stars. We fit a synthetic model to detailed stellar evolution models in the mass range 9<=M/Msun<=11.5 (Z=0.02), and extrapolate these fits to the end of the AGB. We determine the number of thermal pulses and AGB lifetime as a function of mass and mass-loss prescription. Our preliminary nucleosynthesis calculations show that, for a reasonable mass-loss rate, the effect of hot-bottom burning in super-AGB stars on the integrated yield of a stellar population is not large. There are many uncertainties, such as mass-loss and convective overshooting, which prevent accurate yield calculations. However, as potential progenitors of electron-capture supernovae, these stars may contribute 7% of non-type-Ia supernovae." @default.
- W1691799114 created "2016-06-24" @default.
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- W1691799114 date "2006-03-28" @default.
- W1691799114 modified "2023-09-27" @default.
- W1691799114 title "Synthetic Super AGB Stars" @default.
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- W1691799114 hasPublicationYear "2006" @default.
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