COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2693 Konkoly Observatory Budapest 25 March 1985 HU ISSN 0374 - 0676 PHOTOELECTRIC TINES OF MINIMUM LIGHT OF HI PUPPIS The first photoelectric observations of HI Puppis (= CoD -49d2909 = CPD -49d1276 = S 4884 ) were obtained in January, 1981 with the 0.6-m telescope at Cerro Tololo Inter-American Observatory in Chile. Differential measurements in B and V were made on nine nights resulting in 780 individual observations in each bandpass. Each observation is an average of two ten second integrations. The times of minimum light shown in Table I were determined by an iterative process using the method of Hertzsprung (1928). Photographic epochs of minimum light were previously obtained by Hoffmeister (1956). The O-C values in Table I were computed from the ephemeris Min I (Hel. J.D.) - 2444609.7720 + 0.43256515 E +-0.0025 +-0.00000014 (p.e.) which was derived by a least squares analysis utilizing the photoelectric and photographic data. The times of minimum were weighted 10 to 3, photoelectric to photographic. The observations, period study, and analyses of the light curves are being published separately. Table I. Times of minima for HI Pup ---------------------------------------------- HEL. J.D. MIN EPOCH O-C FILTER ---------------------------------------------- 2444608.69007 II -2.5 0.0005 B,V 2444609.77208 I 0.0 -0.0001 B,V 2444611.71909 II 4.5 -0.0006 B,V 2444614.74561 II 11.5 0.0009 B,V 2444616.69329 I 16.0 -0.0003 B,V ---------------------------------------------- J.R. KERN and BEVERLY B. BOOKMYER Dept. of Physics and Astronomy Clemson University Clemson, SC 29631 U.S.A. References: Hertzsprung, E., 1928, Bull. Astr. Inst. Netherlands 4, 179. [BIBCODE 1928BAN.....4..172H ] Hoffmeister, C., 1956, Veroff. Sonneberg, 3, (1), 7, 26.