COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1396 Konkoly Observatory Budapest 1978 March 22 KO Aur KO Aur = Wr 122 = BD +48d1340 was discovered by Weber, R. in 1963. He classified this star as an eclipsing binary (1). Weber also gives the first elements obtaining a period of 0.428949d (2). I observed the star on 117 plates of the Hartha sky-patrol (JD.2437300-38800) and searched on Sonneberg sky-patrol plates. The obtained minima, listed below, show that the elements of Weber are not correct. The following improved elements could be derived: Min.(hel.) = JD.2436607.472+ 1.31793028d E. Observed minima: JD.(hel.) Epoch O-C 2435762.655 - 641 -0.024d 36607.450 0 - .022 37639.459 + 783 + .048 730.356 852 + .007 940.545 1011.5 - .013 38406.478 1365 + .031 495.380 1432.5 - .027 651.610 1551 + .028 849.311 1701 + .040 39070.627 1869 - .057 40205.425 2730 + .003 41592.495 3782.5 - .048 689.379 3856 - .032 957.556 4059.5 - .054 42697.573 4621 - .055 866.368 4749 + .045 870.323 4752 + .046 Using the improved elements the observations of Weber, R. and Diethelm, R.(3) can be exhibited. KO Aur is an eclipsing binary (10.45m-11.30m ph). Comparison stars are published in (1). The secondary minimum seems to be of the same depth as the primary minimum. Further particulars will be published in "Mitteilungen der Bruno-H.-Burgel-Sternwarte Hartha" Heft 12. TH. BERTHOLD Bruno-H.-Burgel-Sternwarte DDR-7302,Hartha References: (1) Weber, R. 1963 Inf.Bull.Var.Stars No. 21 (2) Weber, R. 1964 Bulletin de la station astrophotographique de Mainterne No. 4 p. 15 (3) Diethelm, R. 1976 BBSAG Bull. 26