COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2282 Konkoly Observatory Budapest 1983 February 22 HU ISSN 0374-0676 PHOTOELECTRIC OBSERVATIONS OF W UMa (BD +56deg1400) This well known eclipsing variable has been on the observing list of the Ege University Observatory for the last two years. Observations in two colours, B and V are in progress. The variable was observed in October, 1982 during two (23 and 24) and in November, 1982 during three nights (2, 23, 25). The data for 23 and 24 October had been already reduced and Hel. Min. times were presented (Hamzaoglu, M., Hamzaoglu, E., 1982). Here we present the latest two minima obtained on 23 and 25 November, 1982 both in V colours, where JD Hel Min I=2444986.3624 + 0.33363808d*E were used. So far in the published reports of this star, we presented only the minimum times together with the (O-C) values according to the above given ephemeris. No errors were presented. Any classical method can be used and observations can be fitted to parabola, but asymmetry and seasonal changes within the light curve of the star prevented us in doing so. Instead, we adopted the chord bisection method and applied the least square fit to the mid-points of the minima. We present the journal of data in Table I obtained from the above given ephemeris. Table 1 Date J.D. Hel. Type of Colour E (O-C) days Min 23 Oct.1982 2445266.61735 Min I B 840 -0.00104+/-0.00007 24 Oct.1982 2445267.61805 Min I B 843 -0.00125+/-0.00006 02 Nov.1982 2445276.45917 Min II B 869.5 -0.00154+/-0.00010 23 Nov.1982 2445297.47882 Min II V 932.5 -0.00109+/-0.00010 25 Nov.1982 2445299.47919 Min II V 938.5 -0.00255+/-0.00008 MELEK HAMZAOGLU, FEHMI EKMEKCI and ESAT HAMZAOGLU Ege University Observatory P.K. 21 Izmir - Turkey References: Hamzaoglu, M., 1982 I.B.V.S. No. 2230 Hamzaoglu, E., Keskin, V., Eker, T. 1982 I.B.V.S. No. 2102