Analysis of the light curves of the eclipsing system V548 Cygni

Details Analysis of the light curves of the eclipsing system V548 Cygni Analysis of the light curves of the eclipsing system V548 Cygni

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..77..391e&link_type=abstract

Astrophysics and Space Science, vol. 77, no. 2, July 1981, p. 391-408.

Astronomy and Astrophysics

Astrophysics

2

Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Astronomical Photography, Cygnus Constellation, Electrophotometers, Orbital Elements, Stellar Atmospheres

Scientific paper

The eclipsing binary V548 Cygni was observed photoelectrically in B and V colors on 17 nights in 1975 with a 48 cm Cassegrain telescope. Three times of minima have been obtained and new light elements have been derived. Solutions of the light curves have been obtained using the methods of Kitamura (1965) and Wood (1971, 1972, 1973). The system has a third body whose total luminosity is greater than that of secondary companion.

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