Stabilization of helium shell burning by rotation in accreting white dwarfs

The currently favored scenario for the progenitor evolution of Type Ia supernovae (SNe Ia) presumes that white dwarfs in close binary systems grow to the Chandrasekhar limit via mass accretion from their non-degenerate companions. However, the accreted hydrogen and/or helium usually participate ther...

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Bibliographische Detailangaben

Hauptverfasser:	Yoon, S-C, Langer, N
Format:	Tagungsbericht
Sprache:	eng
Online-Zugang:	Volltext
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