COMMISSION 27 OF THE I.A.U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 121 Konkoly Observatory Budapest 14 February 1966 BV 394 = BD+42deg3471 (8.9m) Observations by R. WEBER, Paris (communication by letter) and K. HAUSSLER (communicated in Hartha Beobachtungs-Zirkular 1966, No. 34, 35, 36) proved our data concerning variability and type of Cepheid of BD +42deg3471 (8.9m) given in Vol. VI, No. 16 of the "Veroffentlichungen der Remeis-Sternwarte Bamberg". According to his observations HAUSSLER had already derived a period on which we based our calculations. Because of the large time-interval covered by our observations we could improve the period and we had to enlarge it from 4.925 249d to 4.925 46d. The period is accurate according to an interval of 2564 epochs (1932-1965). Magnitude-estimations of HAUSSLER have been fitted to our lightcurve. Elements: Max = 2426427.300 + 4.925 46d E (Cep) ptg. magnitudes: 9.4m - 10.3m (Fig. 1) Maxima JD E O - C JD E O - C 242 6427.558 0 +0.258d 242 8752.452 472 +0.335d 6811.522 78 +0.034 9077.449 538 +0.252 .536 78 +0.050 9111.387 545 -0.309 .552 78 +0.066 243 6731.506 2092 +0.144 W ^+/ .572 78 +0.086 6756.462 2097 +0.472 W. .593 78 +0.107 6761.460 2098 +0.445 W. 6860.467 88 -0.273 6780.417 2102 -0.200 W. .488 88 -0.252 6785.421 2103 -0.121 W. .509 88 -0.231 6810.398 2108 +0.228 W. 6949.355 106 -0.044 6815.367 2109 +0.272 W. .376 106 -0.023 6899.250 2126 +0.422 H ^++/ .398 106 -0.001 7199.479 2187 +0.178 H. 7003.255 117 -0.323 7583.294 2265 -0.173 .278 117 -0.301 7903.395 2330 -0.227 7274.398 172 -0.081 7933.319 2336 +0.144 7333.184 184 -0.251 8258.431 2402 +0.176 H. .356 184 -0.229 8322.333 2415 +0.047 H. 7983.490 316 -0.251 8652.473 2482 +0.181 H. .515 316 -0.230 8672.423 2486 +0.429 H. 8067.350 333 -0.128 9002.357 2553 +0.358 H. 8107.292 341 +0.411 9056.292 2564 +0.113 H. 8126.272 345 -0.312 +/ = R. WEBER, communication by letter ++/ = K. HAUSSLER, Harthaer Beobachtungs-Zirkular (HBZ), 1966, No. 34. 35, 36. Bamberg, Remeis-Observatory 1 February 1966 H. OTT