COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 331 Konkoly Observatory Budapest 1969 February 12 FLARES OF YZ CMi OBSERVED AT OKAYAMA 14 TO 16 DECEMBER, 1968 AND 14 TO 25 JANUARY, 1969 A continual photoelectric monitoring of the flare star YZ CMi was done with the 91-cm reflector of the Okayama Station from 14 to 16 December, 1968, and from 14 to 25 January, 1969. The large flare on 14 January 1968, of which the maximum DeltaB was more than 1.8 magnitudes may be the largest one ever observed for YZ CMi. The following Table shows the time of monitoring and the time of flares. Some more details will be published in the Tokyo Astronomical Bulletin. Time of Time of max. Duration Integr. Date Monitoring max. DeltaB intensity 1968 Dec.14d 15h42m-18h15m 17h21.3m> 1.81mag 12min 6min 15 14 49 - 19 30 15 25.5 0.17 0.7 0.1 17 33.5 0.52 6 2 19 12.3 0.24 3.2 0.2 16 13 10 - 13 53 13 46.3 0.41 1.5 0.15 14 04 - 15 09 15 20 - 15 50 1969 Jan.14 14 26 - 15 03 17 47 - 18 16 15 10 20 - 13 04 13 09 - 13 21 16 10 - 16 18 16 26 - 17 50 18 36 - 19 03 18 47.2 0.37 0.3 0.06 17 11 05 - 13 36 16 16 - 18 44 17 31.4 0.92 4 0.7 18 50 - 19 31 19 12 50 - 13 12 16 47 - 16 58 17 13 - 17 19 21 11 09 - 15 09 22 13 30 - 19 00 23 10 00 - 11 56 13 00 - 17 22 16 19.0 0.45 2.4 0.2 Integrated intensity = Intergral((I_flare - I_normal)/I_normal) dt. Tokyo Astronomical Observatory K. OSAWA K. ICHIMURA February 7, 1969. T. NOGUCHI E. WATANABE