COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 3127 Konkoly Observatory Budapest 4 January 1988 HU ISSN 0374-0676 TIMES OF MINIMA OF SOUTHERN ECLIPSING BINARIES As part of an extensive program devoted to search for periods, times of minimum light and period variations of bright southern close binaries, we present here photoelectric minima for RS Sgr, RR Cen, and IT Nor. Observations were made between 1985 and 1987 at the Yale Southern Station of Felix Aguilar Observatory (San Juan, Argentina) with the 76 cm reflecting telescope, refrigerated RCA 31034 photomultiplier and photon counting techniques. The usual symmetrical pattern was followed during the measurements through the filters, in alternative sequences variable-comparison star and sky reading. The following times of minimum were determined: Star Filter Min HJD m.e. 2440000+ RS Sgr V I 6296.5126 0.0048 RS Sgr B I 6296.5120 0.0060 RS Sgr U I 6296.5106 0.0065 RS Sgr V I 6622.6362 0.0006 RS Sgr B I 6622.6356 0.0049 RS Sgr U I 6622.6359 0.0040 RR Cen V I 6621.6678 0.0034 RR Cen B I 6621.6677 0.0041 RR Cen U I 6621.6677 0.0046 IT Nor V I 6623.7370 0.0048 IT Nor B I 6623.7369 0.0074 IT Nor U I 6623.7372 0.0106 IT Nor V II 6624.7151 0.0049 IT Nor B II 6624.7151 0.0047 IT Nor U II 6624.7151 0.0032 A study of the period of RS Sgr and a light curve analysis of IT Nor will be published elsewhere. MIGUEL ANGEL DE LAURENTI MIGUEL ANGEL CERRUTI Observatorio Astronomico Mercedes IAFE Calle 29 No. 575 CC 67 Suc 28 6600 Mercedes (Buenos Aires) 1428 Buenos Aires Argentina Argentina