Abstract
Photoelectric observations, in U, B and V, of the system GO Cygni were obtained during 1995 at the Birouni Observatory, Shiraz, Iran, and the corresponding light curves analysed with the use of Wilson-Devinney;'s techniques. New photoelectric and absolute elements for the system are given. The period of the system, a reverse Algol type semi-detached binary was found to continue its increasing.
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Edalati, M., Atighi, M. Photometric Observations and Light Curves Analysis of Go Cygni. Astrophysics and Space Science 253, 107–117 (1997). https://doi.org/10.1023/A:1000532232009
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DOI: https://doi.org/10.1023/A:1000532232009