Numerical modelling of the classical nova outburst
Copyright policy )Numerical modelling of the classical nova outburst
AbstractWe describe a mechanism that promises to explain how classical nova outbursts take place on white dwarfs of 1 M⊙ or less and for accretion rates of 4 × 10−10 M⊙ yr−1 or greater.
- University of North Texas United States
- National Aeronautics and Space Administration United States
- Los Alamos National Laboratory United States
- Goddard Space Flight Center United States
Numerical Solution, General Physics, Mathematical Models, White Dwarf Stars, Star Evolution, Instability, Explosions, Variable Stars 640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar, Eruptive Variable Stars, Stars, Radio & X-Ray Sources, Dwarf Stars, Plasma Instability, Star Accretion, 71 Classical And Quantum Mechanics, Novae, Plasma Macroinstabilities, Helmholtz Instability
Numerical Solution, General Physics, Mathematical Models, White Dwarf Stars, Star Evolution, Instability, Explosions, Variable Stars 640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar, Eruptive Variable Stars, Stars, Radio & X-Ray Sources, Dwarf Stars, Plasma Instability, Star Accretion, 71 Classical And Quantum Mechanics, Novae, Plasma Macroinstabilities, Helmholtz Instability
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