COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 433 Konkoly Observatory Budapest 1970 April 28 PHOTOMETRY OF AD Leo Over the period 1st to 15th March 1970, observations were made at Boyden Observatory of AD Leo as a part of the International Co-operative Programme. The 40 cm Nishimura Reflector was used in this work fitted with a Johnson B. Filter and a solid CO2 cooled E.M.I. 6256 photomultiplier tube. As evident from the table the monitoring time totalled 41h07m. Three flares were recorded, each of low intensity. Flare No.1 is interesting in that it was of relatively long duration (approximately 13 minutes) similar to the one previously reported (A.H. Jarrett and J.P.Eksteen MNASSA Vol XXVIII, page 70). Monitoring table of AD Leo 1970 U.T. Total Flare U.T. of Duration delta m March hours No. flare per night 1 18.31-19.50,20.54-21.25 1h50m 2 18.18-20.42,21.05-23.00 4 19 1 19h24.4m 12.6m 0.31 3 18.07-23.05,23.22-00.12 5 48 4 20.40-23.48 3 08 5 18.05-21.57,22.04-00.34 6 22 2 14 41.9 5.1 0.30 6 18.01-21.20,21.32-22.32 4 19 3 21 53.2 4.1 0.28 9 17.56-22.45,22.52-00.15 6 12 10 17.47-22.45 4 58 11 17.52-22.03 4 11 Total 41h07m [FIGURE 1] [FIGURE 2] [FIGURE 3] A.H. JARRETT and J.P.EKSTEEN Boyden Observatory University of the Orange Free State Department of Astronomy P.O. Box 334 Bloemfontein Rep.of South Africa