COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2507 Konkoly Observatory Budapest 24 April 1984 HU ISSN 0374-0676 PHOTOELECTRIC OBSERVATIONS OF 1 Per AND BU Tau The two variable stars have been observed in the V-band with a 165/1430 Newtonian telescope. The phases of 1 Per were calculated with the elements from Poretti (1982): Min I = JD 2443562.853 + 25.9359d x E (1) Distinct minimum could only be observed at phase 0.41. 1 Per Delta V are in the sense 4 Per minus 1 Per 4 Per (5.007 V, B8V) Hel. J.D. Phase Delta V Hel. J.D. Phase Delta V 2440000 + 2440000 + 5638.275 0.026 -0.53 5671.217 0.291 -0.57: 5645.279 0.290 -0.47 5673.304 0.368 -0.49 5647.238 0.367 -0.50 5689.213 0.985 -0.42 5648.229 0.405 -0.61 5691.221 0.062 -0.54 5648.279 0.407 -0.63 5751.321 0.380 -0.58: 5651.250 0.521 -0.48 5752.292 0.414 -0.71 5652.238 0.560 -0.50 5759.300 0.688 -0.49 5661.254 0.907 -0.56 5778.292 0.420 -0.67 5663.203 0.983 -0.48 5779.283 0.459 -0.50: 5663.233 0.984 -0.46 5780.279 0.497 -0.52 The variable BU Tau was in maximum light during the observing time. There were small amplitude variations present. BU Tau comparison star: 16 Tau (5.46 V, -0.04 (B-V)) check star: 19 Tau (5.65 V, -0.07 (B-V)) Hel. J.D. Hel. J.D. Hel. J.D. 2440000+ V 2440000+ V 2440000+ V 5346.29 5.10 5645.27 5.20 5691.29 5.17 5406.29 5.13 5647.27 5.22 5705.29 5.16: 5407.30 5.13 5651.30 5.21 5744.25 5.17 5430.31 5.13 5663.25 5.25 5751.29 5.24: 5617.37 5.20 5683.26 5.13: 5759.29 5.23 5621.32 5.25: 5684.28 5.15: 5778.31 5.15 5638.25 5.11: 5689.26 5.22 5780.31 5.13 D. BOHME 4851 Nessa 11 Pf.: 93 German Democratic Republic Reference: Poretti E., 1982, I.B.V.S. No. 2239