COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1079 Konkoly Observatory Budapest 1976 January 2 THE NEW PHOTOMETRIC ELEMENTS OF BS DRACONIS During 1972-1974, 813 photoelectric observations of BS Dra were carried out at the Astronomical Observatory of the University of Cluj-Napoca. The observations were made in V and B light with a 50 cm Newton reflector, a photometer employing an unrefrigerated 1 P 21 photomultiplier tube and Corning 3384 and BG 12 + GG 13 filters, respectively. Table 1 contains the observed times of minima. Using the minima published by Oburka (1971, 1972), Kizilirmak and Pohl (1974) as well as those from Table 1, the following elements have been determined: Min I = J.D.hel.2426444.5834 + 3.363988d E Table 1 -------------------------------------------------- Min.hel. n E O-C Obs. J.D.24... -------------------------------------------------- 41498.4290 49 4475.0 -0.0009 I. Todoran 41508.5199 43 4478.0 -0.0018 I. Todoran 41631.3123 62 4514.5 +0.0056 V. Pop 41772.5934 67 4556.5 -0.0013 V. Pop 41794.4600 34 4563.0 -0.0007 I. Todoran -------------------------------------------------- The real period is twice as long as the value published in G.C.V.S. (1969). The O-C differences calculated with the new elements are also given in Table 1. The general picture of the mean light curve in V is plotted in Figure 1, whence we can see that the secondary minimum occurs at the phase 0.5p. The computation of the orbital elements is in course of preparation, and they will be published elsewhere. Astronomical Observatory DORIN CHIS of Cluj-Napoca, Romania. VASILE POP IOAN TODORAN References: Oburka, O. Contr.Obs.Plan. in Brno 1971, 12, 9 Oburka, O. Contr.Obs.Plan. in Brno 1972, 14, 4 Kizilirmak, A., Pohl, P. I.B.V.S. 937, 1974 [FIGURE 1]