Место издания:Astronomical Society of the Pacific [Provo, Utah, etc.], United States
Первая страница:237
Последняя страница:239
Аннотация:We present UBV(RI)C photometry of the classical novae V339 Del and
V2659 Cyg. The U-band data of the fast nova V339 Del were used to find a possible
orbital period of 0.1314 d. The time of a two-magnitude decline from maximum, t2,V =
65 days, was used to determine the basic parameters of the slow nova V2659 Cyg.