A probable non-degenerate H-burning flash on the white dwarf of the symbiotic slow nova V 1329 Cygni

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Binary Stars, Novae, Symbiotic Stars, White Dwarf Stars, Emission Spectra, Giant Stars, Light Curve, Planetary Nebulae, Stellar Luminosity, Stellar Spectrophotometry

Scientific paper

We review the entire photometric history of V 1329 Cyg and present a set of new B and V magnitudes spanning 4.5 years or almost 2 complete orbital cycles. Taking also advantage of the extensive IUE data in the literature, we derive a number of observational constraints to which every interpretative model must be confronted. We then use these constraints to propose our interpretation of V 1329 Cyg, in terms of a non-degenerate H-burning flash on a luminous white dwarf. Its validity is anyway clearly separated in the text from the experimental evidence of the constraints derived from analysis of the photometric history.

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