The symbiotic nova PU VUL

Details The symbiotic nova PU VUL The symbiotic nova PU VUL

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.236..113s&link_type=abstract

In ESA Recent Results on Cataclysmic Variables p 113-115 (SEE N86-20287 10-93)

Physics

2

Novae, Stellar Evolution, Symbiotic Stars, Brightness, Stellar Envelopes, Stellar Luminosity, Stellar Models, Stellar Oscillations

Scientific paper

An evolutionary scenario for PU Vul (Kuwano-Honda object) behavior
beginning from 1978 is discussed. The star is identified as a very slow
nova. It passed through phases of outburst, almost constant brightness
with small amplitude quasiperiodic oscillations, and expansion of the
dusty envelope.

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