COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 453 Konkoly Observatory Budapest 1970 July 20 PHOTOELECTRIC TIMES OF MINIMA OF RR CENTAURI The eclipsing binary RR Centauri = HD 124689 has been observed photoelectrically at the Bosque Alegre Station of the Cordoba Observatory. The observations were taken at the 154 cm reflecting telescope with a RCA lP28 photomultiplier plus a GG14 Schott glass filter. The photoelectric signals were amplified through a Field Effect Transistor amplifier (Sistero, 1970). The primary minimum was observed on June 24 about U.T. 2 20m. From 69 peV observations the time of primary minimum was derived: Min. I. = J.D. hel 2440761.6003 +- 0.0028 m. e. and from 80 observations on June 25 the time of secondary minimum was obtained: Min.II. = J.D. hel 2440762.5158 +- 0.0014 m.e. From the observed times of minima new light elements were derived by comparisons with the elements in the finding list given by Koch, Sobieski and Wood (1963). The Knipe's elements given there, compared with the present observations, permit an improved re-determination of the period: P = 0d60569131 +- 0d00000058 m.e. Table I lists the minima with the given weights and the cycles and residuals from the linear light elements: Min.I = J.D. hel 2438946.9535 +- 0.60569131. E 0020 +- .00000058 m.e. We are continuing work on this star. TABLE I. Min J.D. hel E W O-C I 2437132.3014 -2996 4 -0.001d I 2440761.6003 +2996 1 -0.004 II 2440762.5158 +2997.5 3 +0.003 R.F. SISTERO M.E. CASTORE de SISTERO Cordoba Observatory Laprida 854, Cordoba Argentina References Koch, R.H., Sobieski, S. and Wood, F.B. 1963, Pub. of the Univ. of Pennsylvania, Astr. Series Vol.IX. Sistero, R.F., 1970, in preparation.