COMMISSION 27 OF THE I.A.U. INFORMATION BULLETIN ON VARIABLE STARS Number 2985 Konkoly Observatory Budapest 17 February 1987 HU ISSN 0374 - 0676 PHOTOELECTRIC OBSERVATION OF THE FLARE STAR UV Cet IN DECEMBER 1985 The flare star UV Cet was monitored in cooperation with EXOSAT program on December 22, 1985 from 16h19m to 18h49m UT and on December 23 from 16h46m to 20h01m UT using the 1.25 m Cassegrain telescope with a five-channel photon- counting UBVRI-photometer. The UBVRI bands are close to the Johnson standard system, 2 sec integration time and 20" diaphragm were used. During the first night no flare activity was observed, see Fig. 1 where records of star+background and background only are shown. [FIGURE 1] Note that a flare limit detection in a single integration is 0.3 mag at the 1 sigma level. During the second night rather high flare activity was observed: five flares are recorded and they are shown in Fig. 2. [FIGURE 2] A clear preflare is observed before the last, the most powerful flare. Few characteristics of the recorded flares are given in Table I : Table I N UT_max t_a t_b P Delta m_u 23/12/85 1 16h50m.5 0.5 4.2 6.2 1.2 2 17h00m.9 1.5 2.5 4.5 1.3 3 17h38m.7 0.3 3.2 9.4 2.1 4 17h42m.3 0.5 3.8 6.1 0.9 5 18h56m.1 0.2 2.5 7.8 3.2 a. The universal time of the flare maximum, UT_max. b. The flare duration before and after its maximum, t_a and t_b (min). c. The equivalent duration of the flare, P (min). d. The amplitude of the flare in U-band, Delta m_u. I.V. ILYIN Crimean Astrophysical Observatory 334413 Nauchny, Crimea U.S.S.R.