Three-Dimensional Simulations of Core Ignition in Sub-Chandrasekhar Mass Models
- 1 January 1997
- book chapter
- Published by Springer Nature
Abstract
No abstract availableKeywords
This publication has 12 references indexed in Scilit:
- Simulations of brittle solids using smooth particle hydrodynamicsComputer Physics Communications, 1995
- Oxgen-burning hydrodynamics. 1: Steady shell burningThe Astrophysical Journal, 1994
- Smoothed Particle HydrodynamicsAnnual Review of Astronomy and Astrophysics, 1992
- Numerical simulations of off-center detonations in helium shellsThe Astrophysical Journal, 1991
- Successive detonations in accreting white dwarfs as an alternative mechanism for type I supernovaeThe Astrophysical Journal, 1990
- Dynamic mass exchange in doubly degenerate binaries. I - 0.9 and 1.2 solar mass starsThe Astrophysical Journal, 1990
- Three-dimensional hydrodynamical simulations of stellar collisions. II - White dwarfsThe Astrophysical Journal, 1989
- The Physics of Supernova ExplosionsAnnual Review of Astronomy and Astrophysics, 1986
- The (N-14) (e-, nu) (C-14)(alpha, gamma)(O-18) reaction and helium flashes in accreting helium white dwarfsThe Astrophysical Journal, 1986
- Accreting white dwarf models of Type I supernovae. III - Carbon deflagration supernovaeThe Astrophysical Journal, 1984