CARBON SHELL OR CORE IGNITIONS IN WHITE DWARFS ACCRETING FROM HELIUM STARS
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/821/i=1/a=28/pdf
Reference42 articles.
1. The dependence of the evolution of Type Ia SN progenitors on the C-burning rate uncertainty and parameters of convective boundary mixing
2. THE C-FLAME QUENCHING BY CONVECTIVE BOUNDARY MIXING IN SUPER-AGB STARS AND THE FORMATION OF HYBRID C/O/Ne WHITE DWARFS AND SN PROGENITORS
3. Hybrid C–O–Ne white dwarfs as progenitors of Type Ia supernovae: dependence on Urca process and mixing assumptions
4. Three-dimensional pure deflagration models with nucleosynthesis and synthetic observables for Type Ia supernovae
5. On the Evolution of Stars that Form Electron‐Degenerate Cores Processed by Carbon Burning. III. The Inward Propagation of a Carbon‐Burning Flame and Other Properties of a 9M☉Model Star
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