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Binary Interaction Dominates Mass Ejection in Classical Novae
Ken J. Shen,
Eliot Quataert
Astrophysical Sciences
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peer-review
18
Scopus citations
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Keyphrases
Optically Thick
100%
Mass Ejection
100%
Classical Novae
100%
Binary Interaction
100%
White Dwarfs
80%
Mass Loss
80%
Low-mass
20%
Hydrodynamic Simulation
20%
Physical Processes
20%
Pressure Control
20%
Cataclysmic Variables
20%
Radiation Pressure
20%
Stellar Evolution
20%
Outburst
20%
Two-mode
20%
Aspherical
20%
Acceleration Zone
20%
Ejecta
20%
Novae
20%
Physics
White Dwarf
100%
Classical Novae
100%
Hydrodynamical Simulations
25%
Physical Process
25%
Cataclysmic Variables
25%
Radiation Pressure
25%
Stellar Evolution
25%
Optical Bursts
25%
Ejecta
25%
Novae
25%