COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2083 Konkoly Observatory Budapest 1982 February 8 HU ISSN 0374-0676 TWO (O-C) RESIDUALS OF W URSAE MAJORIS SYSTEM The well known short period (0.333d 63808) eclipsing variable, W Ursae Majoris (BD+56d1400) was observed with a photoelectric photometer attached to the 48 cm Cassegrain telescope at the Ege University Observatory, Izmir. The observations were carried out on January 16-17, 1982 on two nights of excellent sky conditions, which are rare for this time of the year. The first night complete light curve and the second night the primary minimum were obtained. On both nights the (BD+56d1399, 8.5m) star was monitored as a comparison star with EMI 9781 A as a detector. [FIGURE 1] Fig.1: Two primary minima of W UMa obtained on 16-17 Jan., 1982 The star is well known for the variation of its orbital period and there are observational evidences for the oscillatory variations within the (O-C) residuals. Also there are some other indications of the second oscillatory variations superimposed on the (O-C) residuals. We shall present a discussion somewhere else on these oscillatory variations of the (O-C) residuals. Our (O-C) values are, (O-C)_1= -0.005d = -7.27m (January 16,1982)-(O-C)_II 0.0053=7.63m (O-C)_2= -0.0045d= -6.48m (January 17,1982) for which, Hel Min I= JD 243 7986.9742+0.33363808d.E was adopted. On the other hand our accurate observed time of primary minimum are: JD_1 = 244 4986.3624; JD_II= 244 4986.5290 JD_2 = 244 4987.3639 Acknowledgements We would like to express our gratitude to Mr. E. Kucuktaka and to Mr. O. Tumer for their help. E. HAMZAOGLU, V. KESKIN and T. EKER Ege University Department of Astronomy Bornova-Izmir Turkey References: Mikolajewska, J. and Mikolajewski, M., 1980, IBVS No. 1812. Rucinski, S.M., Gondhalekar, P., Pringle, J.E. and Whelan, J.A.J., 1980, IBVS No. 1844.