High-speed photometry of symbiotic stars and recurrent novae

Details High-speed photometry of symbiotic stars and recurrent novae High-speed photometry of symbiotic stars and recurrent novae

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mnras.179..587w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 179, June 1977, p. 587-594.

Astronomy and Astrophysics

Astronomy

26

Binary Stars, Mass Transfer, Novae, Stellar Luminosity, Stellar Models, Stellar Spectrophotometry, Giant Stars, Hot Stars, Light Curve, Signal To Noise Ratios

Scientific paper

High time resolution photometry of 12 southern symbiotic stars shows that there is no flickering activity, in contrast with the recurrent novae where the flickering amplitude may reach several tenths of a magnitude. If a binary star model is used to explain the properties of these stars then the constancy of the symbiotic stars is a consequence of the mass transfer rate being lower than for the recurrent novae.

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