COMMISSION 27 OF THE I. A. U INFORMATION BULLETIN ON VARIABLE STARS NUMBER 267 Konkoly Observatory Budapest 1968 April 12 YZ CMi A continual photoelectric monitoring of the flare star YZ CMi was done with the 91-cm reflector of the Okayama Station from January 22 to February 6, 1968, by the request of the Working Group of UV Ceti type Stars. - During the 48 hours of monitoring in total, 11 flares were observed as shown in the following Table. - Some more details including the photographs of the recorder charts are published in the Tokyo Astronomical Bulletin, Second Series No. 180. Table 1. Flares of YZ CMi observed at Okayama Jan. 22 to Feb. 6, 1968 Time of Flares Date Monitoring Time of Max. delta m (B) Duration Jan. 22 10^h50^m -12^h41^m 13 06 -14 18 24 16 09 -16 13 16 17 -16 25 17 03 - 19 00 17^h22.5^m 0.22^mag 4^minutes 17 34.2 0.17 3 17 56.7 1.56 12 25 10 11 -11 08 11 12 -11 17 12 00 -15 26 12 53.2 0.38 5 13 42.7 0.23 3 18 07 -18 29 26 10 17 -17 48 18 11 -18 58 27 10 03 -11 39 14 20 -15 03 28 11 07 -14 41 Jan. 30 15 13 -18 26 18 36 -19 17 31 9 43 -10 10 10 10 -15 20 12 23.4 =0.35 ? 12 45.5 >0.35 ? 15 32 -16 10 Feb. 1 14 05 -14 34 2 10 26 -17 30 15 58.9 0.29 2 5 10 01 -12 59 10 45.0 1.39 14 11 20.0 1.32 10 12 14.9 0.30 3 13 07 -14 07 16 08 -16 54 6 13 57 -14 42 17 36 -18 10 K. OSAWA K. ICHIMURA T. NOGUCHI E. WATANABE Tokyo Astronomical Observatory March 22, 1968.