COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2595 Konkoly Observatory Budapest 28 September 1984 HU ISSN 0374 - 0676 PHOTOELECTRIC MINIMA TIMES OF ER ORIONIS The short period (P = 0.4234d) eclipsing binary ER Orionis was observed photoelectrically during 1982 and 1983. The observations were made using the two-beam, multi-mode, nebular-stellar photometer attached to the 48 inch Cassegrain reflector at the Kryonerion Astronomical Station of the National Observatory of Athens. During our observations six new minima times were obtained. They are presented in the following Table, the successive columns of which give: the Hel. J.D. of the six minima, the residuals (O-C), the mean error sigma and the type of minimum. Table I Hel.J.D. (O-C) sigma Min. 2440000+ days days Type 5310.4163 -0.0277 +-0.0003 I 5311.4771 -0.0244 +-0.0004 II 5312.3233 -0.0250 +-0.0004 II 5312.5322 -0.0278 +-0.0003 I 5380.2774 -0.0268 +-0.0003 I 5667.5369 -0.0248 +-0.0004 II The residuals (O-C) have been computed using Kukarkin's et al. (1976) ephemeris formula: Min I = (Hel.J.D.) 2436508.7851 + 0.4234009d E while the times of minima and the mean errors have been calculated using Kwee and Van Woerden's method (1956). P. ROVITHIS H. ROVITHIS-LIVANIOU National Observatory Astronomy Department of Athens, Athens 11810 Athens University Greece Panepistimiopolis GR-157 71 Zografos Greece References: Kukarkin, B.V. et al., 1976, Third Suppl. to the third Edition of the General Catalogue of Variable Stars, Moscow. [BIBCODE 1976tstt.book.....K ] Kwee, K.K., and Van Woerden, H., 1956, Bull. Astr. Inst. Neth., 12, 327. [BIBCODE 1956BAN....12..327K ]