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- W174928478 abstract "The effects of rotation in progenitor models for Type Ia supernovae are addressed. After discussing processes of angular momentum transport in carbon+oxygen white dwarfs, we investigate pre-explosion conditions of accreting white dwarfs. It is shown that differential rotation will persist throughout the mass accretion phase, with a shear strength near the threshold value for the dynamical shear instability. It is also found that rotational effects stabilise the helium shell source and reduce the carbon abundance in the accreted envelope." @default.
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- W174928478 date "2004-12-16" @default.
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- W174928478 title "Type Ia progenitors: effects of spin-up of white dwarfs" @default.
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- W174928478 doi "https://doi.org/10.1017/cbo9780511536236.011" @default.
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