COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 349 Konkoly Observatory Budapest 1969 May 5 PHOTOELECTRIC OBSERVATIONS OF UV Ceti As part of the UV Ceti international patrol the star was monitored at the Boyden Observatory during eight nights in October 1968. The 16" Nishimura reflector was used, fitted with a standard Johnson B-filter and an EMI photomultiplier tube cooled with solid carbondioxide. The phototube output fed directly into a Hewlett Packard type DY-2460A amplifier. As will be seen from Table I, 18 events were recorded with a total of 23 maxima over an observing time of approximately 30 hours. Inclement weather prevented further observations. Delta m is considered accurate to within 5%, spurious or instrumental flares being eliminated. Flare activity was absent on two of the nights during the observation period, but on the night of 24-25 October enhanced activity was evident as a flare rate of one per hour, bringing the number for that night up to 8 with 10 maxima. The flares had 4 typical characteristics of UV Ceti type flare stars. Additionally, about 30% of them showed a rapid decline after the flash phase followed by a secondary maximum and a gradual decline. A note (1) concerning these observations has been published. Ref. (1) J.P. EKSTEEN, MNASSA, 27, 145, 1968. A.H. JARRETT and J.P. EKSTEEN Boyden Observatory, Bloemfontein Rep. of South Africa TABLE I. UV Ceti Monitoring Time and Observed Flares Date Total Flare UT Duration Delta m October UT Hours no. of Min. 1968 Per Night maximum 13 19.47-22.12, 22.44-23.40 3h21m 1 20h29*5 8 0.20 2a 22 52 7 2 0.23 2b 22 55 4 8 0.70 3 23 08 5 3 0.86 4 23 22 0 7 0.81 14 20.34-22.18, 22.26-23.52 3 02 15 20.15-21.39 1 24 19 17.37-21.11, 22.07-23.12 4 39 5 19 29 6 3 0.44 6 20 00 3 3 0.44 23 22.03-22.30, 22.39-0.00 1 51 7 23 10 8 7 0.44 24 0.00-01.30, 17.34-23.33, 23.47-0.00 7 47 8 01 03 9 1.5 0.41 9 18 23 1 18 0.54 10a 19 31 5 9 0.61 10b 19 39 3 0.90 11 19 41 9 3 0.39 12a 20 43 3 3 0.52 12b 20 46 9 2 0.52 13a 22 41 2 3 0.64 13b 22 46 9 3 0.46 14 23 08 3 3 0.28 25 0.00-01.06, 20.7.3-21.29, 21.39-23.42 4 17 15 20 48 3 2 1.00 27 20.54-21.23, 21.37-21.47, 21.57-22.18, 22.24-22.46, 23.00-0.00 2 16 16a 23 43 5 1 0.30 16b 23 45 0 3 0.19 28 0.00-01.11 1 11 17 0 21 4 3 0.49 18 0 37 0 6 0.35 TOTAL: 29H43M (8 nights out of a 16-night period) [FIGURE 1] [FIGURE 2] [FIGURE 3] [FIGURE 4] [FIGURE 5]