COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 3435 Konkoly Observatory Budapest 23 February 1990 HU ISSN 0374 - 0676 PHOTOELECTRIC MINIMA OF ECLIPSING BINARIES Photoelectric observations of the eclipsing binaries 44i Boo, RZ Cas, U Cep and U Sge have been made with the 0.5-m reflector at the Odessa Observatory for the purpose of determining times of minima for the period studies. The comparison stars were GC 20111 for 44i Boo, GC 3075 for RZ Cas, HD 6006 for U Cep and HD 180242 for U Sge. The moments of minima were determined by the chord bisection method for 44i Boo, RZ Cas and by the mean light curve method for U Cep, U Sge. The heliocentric times of the observed minima in yellow filter are given in Table I, along with the epoch number (E), the O-C values and the number of estimates used for each minimum (n). Table I Star Min HJD E O-C n 44i Boo 2447359.3920 28030 +0d0221 10 364.3469 28048.5 +0.0224 20 355.4180 28052.5 +0.0223 14 371.4438 28075 +0.0222 14 375.3270 28089.5 +0.0220 15 388.3163 28138 +0.0223 19 393.4050 28157 +0.0225 33 RZ Cas 370.5336 25112 -0.0554 19 376.5099 25117 -0.0554 22 382.4868 25122 -0.0547 26 394.4394 25132 -0.0547 25 U Cep 361.2810 15833 +0.8922 26 366.2650 15835 +0.8904 28 U Sge 383.5632 8949 +0.0002 27 390.3250 8951 +0.0008 29 The O-C values have been calculated from the ephemeris: 44i Boo Min I HJD = 2439852.4903+ 0.2678159d E RZ Cas Min I HJD = 2417355.4233+ 1.1952519d E U Cep Min I HJD = 2407890.2957 + 2.4929005d E U Sge Min I HJD = 2417130.4090 + 3.3806184d E I thank the Director and the staff of the Odessa Observatory for observing time and assistance. L.P. SURKOVA The Teachers Training College, Chita 672045, USSR