A photometric study of the eclipsing binary V478 Cygni

Details A photometric study of the eclipsing binary V478 Cygni A photometric study of the eclipsing binary V478 Cygni

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26as...53..363s&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 53, Sept. 1983, p. 363-372. Research supported by the Scient

Astronomy and Astrophysics

Astrophysics

7

Astronomical Photometry, Eclipsing Binary Stars, Electrophotometry, Light Curve, Stellar Spectrophotometry, Computerized Simulation, Periodic Variations, Stellar Magnitude, Tables (Data), Variable Stars

Scientific paper

Nearly 1100 new photoelectric observations of the photometrically neglected eclipsing binary V478 Cygni in blue and yellow colours are presented. The improved light elements are calculated from the new photoelectric minima. The light curves were analyzed using D.B. Wood's model simulation program WINK. The system was found to be a detached binary.

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