We have photometrically observed HD 112859, HD 144110, and
HD 208472 using the 48-cm Cassegrain reflector with an SSP-5 photometer of Ege
University Observatory during the 1996Ð1997 observing seasons. Observations
were made between June 1996 and March 1997 using B, V, and R filters and light
curves with color variations were obtained. The amplitudes of the light variations
have been estimated as approximately 0.05, 0.06, and 0.20 magnitude for
HD 144110, HD 112859, and HD 208472, respectively, but considerable scattering
is seen among all the phases.