Abstract
Photoelectric differentialB andV magnitudes of the eclipsing binary V1425 Cygni are presented yielding the complete photoelectric light curve of this relatively bright system. The improved light elements are calculated using the least-squares method.
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References
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Tate, R. C.: 1970,Inf. Bull. Var. Stars, No. 438.
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Güdür, N., Gülmen, Ö., Sezer, C. et al. Photoelectric photometry of the eclipsing binary V1425 Cygni. Astrophys Space Sci 146, 283–297 (1988). https://doi.org/10.1007/BF00637578
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DOI: https://doi.org/10.1007/BF00637578