Photometry and analysis of the eclipsing variable GO Cygni

Details Photometry and analysis of the eclipsing variable GO Cygni Photometry and analysis of the eclipsing variable GO Cygni

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.203..121s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 203, no. 1, p. 121-133.

Astronomy and Astrophysics

Astrophysics

7

Astronomical Photometry, Binary Stars, Light Curve, Mass Ratios, Variable Stars, Astronomical Spectroscopy, Space Observations (From Earth), Stellar Luminosity

Scientific paper

Photoelectric observations of the eclipsing binary GO Cyg have been carried out in B and V colors at the Ege University Observatory. The corresponding light curves were analyzed by the method of Wilson-Devinney. The system was found to be a reverse Algol semi-detached binary. The absolute elements of the system are also deduced.

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