COMMISSION 27 OF THE I. A. U INFORMATION BULLETIN ON VARIABLE STARS NUMBER 226 Konkoly Observatory Budapest 25 September 1967 PHOTOELECTRIC MINIMA AND NEW ELEMENTS FOR V477 CYG From 1963 to 1967 we obtained at the Nurnberg Observatory 5 photoelectric minima of the eclipsing variable V477 Cyg, which show large, increasing O-C's against the elements in GCVS (I) and SAC 38 (II). The period, given in GCVS (1958) and SAC 38 (1967), was derived by Wallenquist immediately after the discovery of the variability of V477 Cyg in 1957. The new elements (III), calculated from the Nurnberg observations with the method of least squares, give a considerable shorter period. Min: J.D. 2432846.2445+2.^d347016*E (I) Min: J.D. 2438650.370+2.347016*E (II) Min: J.D. 2437317.2764+2.3469876*E (III) Minima Observer O-C (I) O-C (II) O-C (III) J.D. 243... 7317.277 vis Pohl -0.^d033 +0.^d012 +0.^d001 8258.417 pe Gorz, Gerhart -0.046 -0.001 -0.001 8664.448 pe Fleischer, Renz -0.049 -0.004 +0.001 8941.392: pe Held, Pohl -0.053: -0.008: 0.000: 9692.4283 pe Bickel, Pohl -0.062 -0.017 0.000^1) ^1) combined with observations on J.D. 2439685. Nurnberg Observatory E. POHL 85 Nurnberg, Lutzowstr. 10 Western Germany PHOTOELECTRIC OBSERVATIONS OF NOVA DELPHINI (II) Stokes Observatory, 1P21 phototube, yellow filter. Hudson, Ohio Date J.D. Magn. Date J.D. Magn. 1967 2439... 1967 2439... Aug. 13 716.7 5.34 Sept. 1 735.6 4.96 Aug. 31 734.6 4.94 Sept. 5 739.6 4.99 Lovell Observatory, 1P21 Phototube. Chagrin Falls, Ohio Date J.D. Magn. Date J.D. Magn. 1967 2439... 1967 2439.. Aug. 13 716.7 5.36 Aug. 26 729.6 5.11 Aug. 14 717.7 5.49 Aug. 28 731.6 4.98 Aug. 22 725.6 5.23 Aug. 29 732.6 4.91 Aug. 23 726.6 5.24 Aug. 31 734.6 4.97 The comparison star for both sets of observations was G.C. 28766 (5.^m9 A0). ARTHUR J. STOKES Hudson, Ohio U.S.A.