COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 340 Konkoly Observatory Budapest 1969 March 29 PHOTOELECTRIC OBSERVATIONS OF AD Leo The results of photoelectric observations of the flare star AD Leo made as a part of cooperative programme in the period of 10-24 February 1969 are given below. The observations were obtained in the B-band with the 64 cm meniscus telescope. The total coverage is 33.3 hours. The content of Tables I, II is identical with those of papers (1) and (2). The light curves of flares (Figs.1, 2,3) are given in relative intensities. P.F. CHUGAINOV N.I. SHAKHOVSKAYA Crimean Astrophysical Observatory [References] (1)P.F. Chugainov, (Photoelectric observations of UV Cet and YZ CMi), I.B.V.S. No. 338, 1969 (2)N.I. Shakhovskaya, (Photoelectric observations of YZ CMi), I.B.V.S. No. 339, 1969 Table I Date Coverage (U.T.) 1969 February 15 19h20m-19h10m, 19h23m-19h26m, 19h33m-20h08m February 16 19h38m -24h00m February 17 0h00m-03h30m February 20 18h11m-18h18m, 18h23m-19h08m, 19h21m-19h24m, 21h08m-21h39m February 21 16h33m-24h00m February 22 00h00m-03h15m, 17h22m-24h00m February 23 00h00m-03h15m Table II Durations Date before Integrated Air of flare and after Deltam Deltam_lim intensity mass maximum maximum, minutes tb ta Feb.16 22h33.3m 0.9 17 0.33 0.017 1.77 1.10 Feb.16 23h11.5m 1.0 6 0.16 0.014 0.22 1.13 Feb.17 01h24.6m 0.2 5 0.16 0.018 0.24 1.44 Feb.17 02h00.4m 0.2 2 0.09 0.018 0.07 1.64 Feb.21 23h33.5m 1.7 8 0.12 0.020 0.51 1.18 Feb.22 17h30.5m 0.2 1 0.39 0.030 0.12 1.92 Feb.22 18h36.6m 1.0 11 0.84 0.020 1.99 1.46 Feb.23 01h00.2m 0.2 12 0.57 0.050 1.29 1.44 [FIGURE 1] [FIGURE 2] [FIGURE 3]