COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 451 Konkoly Observatory Budapest 1970 July 17 YZ CANIS MINORIS Photoelectric monitoring of YZ CMi was carried out at the Auckland Observatory with the 50 cm reflector. The observations were made with an E.M.I. type 9502 photomultiplier tube and a standard B filter. The photometer uses a capacitor integrating circuit to convert the photomultiplier current into a square wave pulse whose frequency waves in proportion to intensity. This is monitored with a digital frequency meter in ten second integrating periods. During 17 hours of monitoring three flares were observed. Table 1 lists monitoring times with remarks on seeing conditions. The details of observed flares are given in Table 2. Table 1. Date Monitoring time Remarks 1970 U.T. Jan.31 1234-1245; 1331-1335 Haze. 1414-1416. Feb. 1 0946-0949; 0950-1032 Clouds and haze at beginning; 1036-1115; 1123-1203 clearer for rest of night. 1217-1244; 1247-1303 1305-1322. 2 1044-1115; 1117-1120; Cirrus 3 1147-1216; 1218-1227; Passing clouds 1259-1302; 1309-1324; 4 0920-0936; 1038-1057; Cloudy with clear patches 5 0906-0911; 0936-0957; Some cloud 1013-1027; 1027-1037; Clear 1039-1104; 1125-1136; 1140-1201; 1214-1243; 1250-1345; 1413-1446; 1454-1526; 1539-1552. 6 1021-1056; Cloudy. 1104-1108; 1112-1126; Clear 1128-1146; 1148-1200; 1209-1233; 1317-1319; Cloudy 7 1028-1045; 1046-1104; Broken cloud 1107-1116; 1258-1321; 1325-1348. 8 0944-0945; 0955-1025 Scattered cloud. 1033-1100; 1111-1129; 1130-1132; 1139-1153; Clear 1156-1200 Clear 1246-1247 Cloud 11 1128-1141 Cloud 1248-1317; 1321-1335; Clear 1337-1351; 1357-1400; 1405-1500; 1512-1523; [FIGURE 1] Times of maxima are + 6 seconds. d_h= duration of flare before maximum; d_a= duration of flare after maximum; S.D. - Standard deviation near flare in B; Max. Mag.= Intensity of max. in B as defined in IBVS 326; Integ. Intensity = Integrated intensity, in minutes, as defined in IBVS 326. The first two flares are depicted in Figures 1 and 2. The commencement of the third flare was not observed. V.S.S. RASNZ FRANK BATESON 18 Pooles Road B.F. MARINO; W.S.G. WALKER Greerton Tauranga New Zealand Table 2. Observed flares of YZ CMi Date Max d_b d_a S.D. Max. Integ. Mag. Intensity B mins. Febr.1 10h22m38s <20^s 3m15s 0.023 >0.42 0.537 6 11 13 35 23 45 0.027 0.19 0.080 7 12 58 10 ? >10mins 0.030 >0.34 - YZ CANIS MINORIS During the 1970 International period YZ CMi was monitored visually by members of the Variable Star Section, RASNZ., as under. No definite flares were observed. Date 1970 Monitoring times U.T. U.T. Jan. 31 09h08m - 09h18m 10 03 - 10 20 10 23 - 11 53 Feb. 1 11 20 - 11 50 12 50 - 13 10 2 10 00 - 10 10 10 32 - 10 37 11 57 - 12 02 3 11 57 - 12 12 12 17 - 12 22 4 09 57 - 10 40 12 02 - 12 18 5 08 54 - 09 54 10 00 - 11 45 6 09 00 - 10 14 10 16 - 10 17 10 34 - 12 00 9 10 10 - 10 17 10 24 - 11 12 11 13 - 13 03 10 10 25 - 13 56 Total 15h08m FRANK M. BATESON Director, Y.S.S., RASNZ 18 Pooles Road Greerton Tauranga, New Zealand V 645 (PROXIMA) CENTAURI V 645 Cen was monitored at the West Melton Observatory, Christchurch (N.Z.) with the 40 cm reflector. The output of the photometer was recorded on tape. No flares were observed. 1970 (U.T.) Monitoring time U.T. May 31 0900 to 1200 June 10 1040 to 1130 FRANK M. BATESON C. ROWE R. AUSTIN M. CLARK V.S.S. RASNZ 18 Pooles Road Greerton Tauranga, New Zealand