Photometric-Study of the Eclipsing Binary V-1073 Cygni

Photoelectric observations of the eclipsing binary V 1073 Cyg have been carried out in B and V colours at the Ege University Observatory. The light curves were analyzed with the Wilson-Devinney approach. A period study reveals that the orbital period of the system is decreasing at the rate of (3.21 +/- 0.17) second per century.