Abstract
Photoelectric observations of the p Cephei-type variable, KP Persei, made in 1977 and 1978 in Zacatecas and San Pedro Ma stir are presented. The photometry was performed mainly in the B system and some nights also in the UB or UBK A frequency naly photometry was carried out. Three sine-wave components with periods P1 = 0. 201779,P2=0. 198085, and P3 = 0d227099 were found.
