ИСТИНА

Here we present the preliminary results of UBV photoelectric observations of two novae in Cygnus that comes to the outburst in summer 2001. The first one, V2274 Cyg, was discovered in the middle of July near its maximum light or soon after it. The second one, V2275 Cyg, was discovered in August before its maximum. Our early photometry of V2274 Cyg started a few days after discovery and lasted up to the end of August, firstly with the help of UBV photometer and with CCD photometer on the 60 cm telescope when it become too faint. A series of observations of V2275 Cyg were made during the autumn of 2001 with UBV photometer on the same telescope. The light curves of these two Novae were derived on the base of our observations and were compared. Classification of both Novae are also considered.