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Smoothed particle hydrodynamics simulations of the core-degenerate scenario for type Ia supernovae
G. Aznar-Siguán
, E. García-Berro
, P. Lorén-Aguilar
, N. Soker
, A. Kashi
Minnesota Institute for Astrophysics
Research output
:
Contribution to journal
›
Article
›
peer-review
33
Scopus citations
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Keyphrases
White Dwarfs
100%
Type Ia Supernovae
100%
Smoothed Particle Hydrodynamics
100%
Circumbinary Disc
66%
Supernovae
33%
Gravitational Waves
33%
Close-enough
33%
Debris
33%
Core Temperature
33%
Three Dimensional Simulation
33%
Overflow
33%
Corona
33%
Asymptotic Giant Branch Stars
33%
Overall Characteristics
33%
Common Envelope
33%
Wave Radiation
33%
Roche Lobe
33%
Highly Eccentric Orbits
33%
Physics
White Dwarf
100%
Type Ia Supernovae
100%
Hydrodynamics
100%
Gravitational Wave
33%
Eccentric Orbit
33%
Roche Lobe
33%
Asymptotic Giant Branch Stars
33%
Supernovae
33%
Electromagnetic Radiation
33%