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Photometric Observation And Period Study of GO Cygni

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arxiv astro-ph/0412627 v3 pith:ZR3GGJWW submitted 2004-12-26 astro-ph

Photometric Observation And Period Study of GO Cygni

classification astro-ph
keywords photometricsystemperiodwereanalysisbandscarriedcurve
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Photometric observations of GO Cyg were performed during the July-October 2002, in B and V bands of Johnson system. Based on Wilson's model, the light curve analysis were carried out to find the photometric elements of the system. The O-C diagram which is based on new observed times of minima suggests a negative rate of period variation (dP/dt<0) for the system.

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