COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1058 Konkoly Observatory Budapest 1975 November 5 SHORT PERIOD VARIABILITY OF NOVA CYGNI 1975 Short period variability of Nova Cygni 1975 was reported by Tempesti (1975a,b) and Koch and Ambruster (1975a,b). Nova Cygni was monitored photoelectrically for about 3 hours in B and V on September 8 and for about 6 hours in V on September 18, 1975. The observations were carried out with the aid of the 60 cm reflector of the Ostrowik station of the Warsaw University Observatory. The star BD +47d3322 was used as the comparison on the first date and BD +47d3340 on the second date. The differences DeltaV and DeltaB (in instrumental system) between the Nova and the corresponding comparison star are plotted in Figure 1. Full dots in Figure 1 denote yellow observations,the open circles correspond to blue observations. The amplitude of light variations was about 0.16 mag. in blue and 0.14 mag. in yellow on September 8 and 0.06 mag. in yellow on September 18. The times of minima determined on basis of the present observations are JD_Hel 2442664.302, 2442674.308 and 2442674.453 and the times of maxima are 2442664.359 and 2442674.359. Figure 2 shows O-C diagram obtained on basis of the present times of minima and maxima and those given by Koch and Ambruster (1975a,b). The times of minima in the Figure 2 are marked with full dots, the times of maxima with open circles. The O-C residuals were calculated with the preliminary ephemeris Min = = 2442664.302 + 0.1410E, Max = 2442664.359 + 0.1410E. The O-C diagram seems to indicate change of period. Thanks are due to Miss J. Wolczyk for help in observations. I. SEMENIUK Warsaw University Observatory References: Koch, R.H., and Ambruster, C.W. 1975a, IAU Circ. 2837 [BIBCODE 1975IAUC.2837....2D ] 1975b, ibid., 2839 [BIBCODE 1975IAUC.2839....1H ] Tempesti, P. 1975a, ibid., 2834 [BIBCODE 1975IAUC.2834....1K ] 1975b, ibid., 2842 [BIBCODE 1975IAUC.2842....1G ] [FIGURE 1] [FIGURE 2]