COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1994 Konkoly Observatory Budapest 1981 July 19 HU ISSN 0374-0676 PHOTOELECTRIC OBSERVATIONS OF BV DRACONIS The short period eclipsing binary BV Dra (SAO 166036) has been observed during August and September 1980 as well as during May 1981. The observations have been made using the two-beam, multi-mode, nebular-stellar photometer of the National Observatory of Athens attached to the 48-inch Cassegrain reflector at Kryonerion Astronomical Station. The B and V filters used are in close accordance to the standard ones. From our observations four primary and six secondary minima times have been derived and are represented Table Hel. J. D. O-C sigma Type of 2444000+ days days Min. 473.4512 0.0127 +-0.0003 II 474.3267 0.0130 +-0.0002 I 475.3781 0.0142 +-0.0003 I 476.4283 0.0142 +-0.0003 I 478.3529 0.0135 +-0.0003 II 480.2772 0.0124 +-0.0003 I 480.4531 0.0133 +-0.0004 II 500.4051 0.0125 +-0.0002 II 506.3578 0.0125 +-0.0002 II 752.4579 0.0168 +-0.0006 II in the following Table. The successive columns give the heliocentric J.D., the residuals O-C, the mean errors sigma, and the type of minimum. The times of minima and the mean errors have been calculated by Kwee and Van Woerden's method (1956) and are the mean values from B and V observations except that at Hel. J.D. 2444480.2772 for which there are observations only in V. The ephemeris used is that of Kukarkin et al. (1969). P. ROVITHIS H. ROVITHIS-LIVANIOU National Observatory of Astronomy Dept, Athens University Athens, Athens 306 Panepistimiopolis, Athens 621 Greece Greece References: Kukarkin, B.V., et al.: 1969, Gen. Cat. of Var. Stars, Moscow. [BIBCODE 1969gcvs.book.....K ] Kwee, K.K. and Van Woerden, H.: 1956, Bull. Astr. Inst. Neth. 12, 327. [BIBCODE 1956BAN....12..327K ]