COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 666 Konkoly Observatory Budapest 1972 April 26 AD Leo The photoelectric monitoring of the flare star AD Leo was carried out at the Okayama Station during the period of 18 to 28 February 1972. The observations were made with the simultaneous three-colour photometer attached to the 91 cm reflector. The observational results are summarized in the Table. Flares Date Time of Filter Time of max. P Duration sigma 1972 Monitoring (UT) max. (UT) Delta m Feb.19d 11h 16m - 12h 16m U 0.71mag 1.8min 5.0min B 11h 21.8m 0.22 0.3 5.0 V - - - - U 0.11^mag U 11 40.5 0.48 0.6 4.5 B 0.02 B 0.09 0.1 4.5 V 0.02 V - - - - 14 19 - 17 00 U 14 15.7 2.70 >8.0 >10 B 0.92 >0.9 >10 V 0.31 >0.3 >6 U 15 31.0 2.56 7.0 15 B 0.88 0.8 15 U 0.16 V 0.29 0.3 15 B 0.03 U 16 45.5 1.98 V 0.03 B 16 45.5 0.57 U >21.4>22 V 16 45.7 0.18 B > 3.2>22 U 16 46.1 1.90 V > 1.2>22 B 16 46.1 0.58 V 16 46.2 0.20 20 10 39 - 12 00 12 26 - 13 00 13 38 - 14 05 15 06 - 15 34 17 07 - 17 36 U 0.92 1.7 4.0 0.16 B 17 29.7 0.20 0.3 4.0 0.05 V 0.05 1.0 1.8 0.02 23 11 07 - 17 11 U 1.47 8.3 15.0 0.20 B 11 33.7 0.41 1.1 15.0 0.03 V 0.15 0.5 14.0 0.02 U 13 47.6 0.62 1.0 7.0 0.16 B 0.10 0.2 5.7 0.03 V 0.04 0.1 0.6 0.02 U 14 59.8 1.27 B 0.22 V 14 59.9 0.08 U 1.25 U 5.7 13.0 0.23 B 15 00.4 0.22 B 0.4 12.0 0.03 V - - V 0.1 4.0 0.02 U 1.13 B 15 00.8 0.21 V - - 28 11 01 - 12 14 13 00 - 18 23 Tokyo Astronomical Observatory 31 March 1972. K. OSAWA, K. ICHIMURA, Y. SHIMIZU, E. WATANABE, T. OKADA, M. YUTANI, H. KOYANO, K. OKIDA