Abstract:
Twelve photoelectric light curves of six eclipsing binary stars namely GG Cas, WX Cep, UZ Cyg, AQ Peg and ST Per in two different filetrs (B and V for the first five binaries and R and I for ST Per) have been analysed by Kopal`s new method of analysis of the light curves of eclipsing system in the frequency domain. The elements of the systems have been evaluated and their evolutionary status discussed