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VARIATION IN THE PERIOD OF THE SYSTEM GO CYG

  • ELKHATEEB M. M. (Department of Astronomy, National Research Institute of Astronomy and Geophysics (NRIAG))
  • Published : 2005.03.01

Abstract

We present a period analysis of the well known $\beta$ Lyrae type eclipsing binary GO Cyg $(P= 0^d .7177)$. Several new times of minimum light, recorded photoelectrically, have been gathered. Analysis of all available eclipse timings of GO Cyg has confirmed a significant period increase with rate of $2.52 {\times} 10^{-10}$ day / cycle, also new period has been estimated. New linear and quadratic ephemerides have been calculated for the system.

Keywords

References

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