Photometric Observation And Period Study of GO Cygni

Details Photometric Observation And Period Study of GO Cygni Photometric Observation And Period Study of GO Cygni

2004-12-26

arxiv.org/abs/astro-ph/0412627v3

Astrophys.Space Sci. 302 (2006) 27-33

Astronomy and Astrophysics

Astrophysics

12 pages, 6 figures, 4 tables, submitted to Ap&SS

Scientific paper

10.1007/s10509-005-9001-z

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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