COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2317 Konkoly Observatory Budapest 20 April 1983 HU ISSN 0374-0676 PHOTOELECTRIC MINIMA TIMES OF THE ECLIPSING BINARY V 508 OPHIUCHI Photoelectric observations of the eclipsing variable star V508 Oph were carried out during 1981. The observations were made using the two-beam, multi-mode, nebular-stellar photometer attached to the 48-inch Cassegrain reflector at Kryonerion Astronomical Station of the National Observatory of Athens. Reduction of the observations was made in the usual way (Hardie, 1962) and the B and V filters used are in close accordance to the standard ones. From our observations three primary and three secondary minima times have been derived using Kwee and Van Woerden's method (1956). They are given in the following Table, the successive columns of which give: the Hel. J.D., the residuals O-C and the type of minimum. The O-C values were calculation Kukarkin's et al. (1976) ephemeris formula: Min.Hel.J.D. = 2428416.339 + 0.34479163d E Table ---------------------------- Hel. J.D. O-C Min. 2444000+ days Type ---------------------------- 783.4265 +0.0012 II 784.4623 +0.0026 II 785.3283 +0.0067 I 785.4958 +0.0018 II 786.3623 +0.0063 I 864.2816 +0.0066 I ---------------------------- P. ROVITHIS H. ROVITHIS-LIVANIOU National Observatory Astronomy Department of Athens, Athens (306) Athens University Greece Panepistimiopolis Athens (621), Greece References: Hardie, R.H.: 1962, Stars and Stellar Systems, Vol. II, "Astronomical Techniques" (Ed.: Hiltner, W.A.), The University of Chicago Press, Chicago, p. 178. Kukarkin, B.V. et al.: 1976, General Catalogue of Variable Stars, Moscow. Kwee, K.K. and Van Woerden, H.: 1956, Bull. Astron. Inst. Neth., 12, 327. [BIBCODE 1956BAN....12..327K ]