A single-star interpretation of Nova Cygni 1975

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Binary Stars, Novae, Stellar Models, Thermonuclear Explosions, White Dwarf Stars, Black Body Radiation, Hydrodynamics, Luminous Intensity, Stellar Mass Ejection

Scientific paper

Observational evidence has revealed that Nova Cygni 1975 is not a
typical nova event. We suggest that Nova Cygni is to be understood, not
in terms of a canonical close binary system, but essentially as a single
star undergoing a thin-shell thermonuclear explosion.

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