Orbital period change during the outburst of the symbiotic binary V 1329 Cygni

Details Orbital period change during the outburst of the symbiotic binary V 1329 Cygni Orbital period change during the outburst of the symbiotic binary V 1329 Cygni

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.201..107h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 201, no. 1, p. 107-112.

Astronomy and Astrophysics

Astrophysics

7

Binary Stars, Orbital Elements, Stellar Orbits, Symbiotic Stars, Novae, Stellar Mass Ejection

Scientific paper

Photographic photometry of the symbiotic nova V 1329 Cygni performed at the Skalnate Pleso Observatory in the years 1979-1991 is presented. An observational proof of the 11.4 d orbital period increase caused by the novalike outburst around 1966 is given. A new ephemeris valid after the year 1971 is as follows: JD(min) = 2446784.862 + 963.306 d x E. The arguments in favor of an accretion-powered outburst are given.

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