COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2410 Konkoly Observatory Budapest 12 October 1983 HU ISSN 0374-0676 ON THE PERIOD OF BW VULPECULAE BW Vul was observed at the Wroclaw Observatory for the World-wide Observing Campaign on BW Vulpeculae organized in 1982 by M.S. Snowden and C. Sterken. The observations were carried out with a 60-cm Cassegrain reflector and a photoelectric photometer equipped with an EMI 6256S photomultiplier tube and a Stromgren b filter. The weather conditions were relatively poor. Our data are, however, sufficiently accurate and numerous to derive a mean epoch of maximum light. Taking the period of BW Vul as equal to P_0 = 0.20103d, and assuming an initial epoch T_0 = 2428000.5, a mean light-curve was derived. It is shown in Figure 1. The points are the individual observations and the solid line, drawn by hand, represents the mean curve. [FIGURE 1] Figure 1 The mean b light-curve of BW Vul. Delta _b_ is the magnitude difference "BW Vul minus a mean of HD 198820 and HD 198527" The following epoch of maximum of BW Vul was derived from the above- mentioned light-curve: Hel. JD (max. light) = 2445228.482d + 0.002d The (O-C) residuals obtained from this epoch of maximum and from the quadratic ephemerides of Valtier (1976) and Margrave (1979) are 0.036d and 0.014d, respectively. On the other hand, the linear ephemeris of Tunca (1978) yields (O-C)= 0.005d. This results indicates that Tunca's two linear ephemerides fit the observations better than the quadratic ephemeris of either Valtier or Margrave. Our observations provide, therefore, another argument in favour of a discontinuous increase of the period of BW Vul. E. SZUSZKIEWICZ AND S. RATAJCZYK Wroclaw University Observatory ul. Kopernika 11 51-622 Wroclaw Poland References: Margrave, T.E., 1979, Publ. A.S.P. 91, 666 [BIBCODE 1979PASP...91..666M ] Tunca, Z., 1978, Inf. Bull. Var. Stars No. 1386 Valtier, J.-C., 1976, Astron. Astrophys. 51, 465 [BIBCODE 1976A&A....51..465V ]