COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 3112 Konkoly Observatory Budapest 18 November 1987 HU ISSN 0374-0676 32 Cyg : UBV PHOTOMETRY OF ECLIPSE IN 1987 The long period eclipsing binary 32 Cyg (V 1488 Cyg) was observed from 6 July to 28 July 1987 during a primary minimum, UBV photometry of this event was obtained using a 0.3 m f/16 Cassegrain telescope and one channel photometer with photomultiplier EMI 9781B. Extinction and transformation coefficients were used to correct the differential magnitudes to the standard system (Hall and Genet, 1982). The comparison star was HD 192985 as suggested by Schroeder (1987). Observations of 32 Cyg are given differentially, with respect to HD 192985. Each value is an average of three individual integrations. Internal errors were +/- 0.01 magnitude. Estimation of amplitude was made from observations in each band : U = 0.68, B = 0.17, V = 0.05. Table I Photometric observations of V1488 Cyg: J.D.(Hel) 2440000+ DeltaU DeltaB DeltaV 6983.482 0m55 -0m56 -1m89 6984.403 0.55 -0.55 -1.90 6986.491 0.59 -0.55 -1.92 6987.439 0.72 -0.55 6988.448 0.79 -0.50 -1.89 6989.554 1.08 -0.48 -1.91 6993.476 1.23 -0.38 -1.85 6996.500 1.02 -0.42 -1.89 6997.451 0.84 -0.49 -1.89 7005.388 0.50 -0.59 -1.88 Time of minimum was determined using tracing paper method (U band), The (O-C) value was calculated using the formula Min(I) = J.D.(Hel) 2444125.96 + 1147.4d E, given by SAC 58 (Cracow). Observed (O-C) Filter J.D,(Hel) Min(I) 2446992.92 -1.04 U Figure 1 shows the light curve in UBV filters from JD 2446983 to 2447005, [FIGURE 1] Figure 1 Primary minimum of V1488 Cyg A. DOLZAN Zasavska 88 61231 Ljubljana Yugoslavia References: Bohme, D., 1987, I.B.V.S. No. 3083 Hall, D.S., Genet, R.M., 1982, Photoelectric Photometry of Variable Stars, I.A.P.P.P. [BIBCODE 1982ppvs.book.....H ] SAC 58, 1986 Cracow Schroeder, K.P., 1987, BAV Rundbrief 36, 61