Circular No. 3397 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. TWX 710-320-6842 ASTROGRAM CAM Telephone 617-864-5758 BD +61 1211 R. Kimble, S. Kahn and S. Bowyer, University of California at Berkeley, report: "We have observed photometrically the suspected RS CVn binary BO +61 1211 = SAO 015338 with the 0.76-m telescope at the Leuschner Observatory. The star has been identified by Liller (IAUC 3176) as the optical counterpart to the x-ray source 2A 1052+606. In 20 nights spread over four cycles of the 7.5-day orbital period (Crampton et al. 1979, submitted to Ap. J.), we see a smooth variation of 0.32 +/- 0.02 mag in V and 0.36 +/- 0.02 mag in B. This photometric variability confirms the classification of the object as an RS CVn system, suggested by Charles et al. (1979, submitted to Nature) on the basis of the observed x-rays and the presence of Ca II H and K emission in the optical spectrum. The epoch of maximum brightness of this unusually large photometric wave is 1979 May 30.1 UT." COMET KOWAL (1979h) E. Helin, California Institute of Technology, communicates the following measurements, by D. R. Janke, of the plates obtained by C. T. Kowal with the 1.2-m Schmidt telescope at Palomar: 1979 UT R. A. (1950) Decl. July 24.21076 19 25 27.50 -17 48 14.8 25.20938 19 24 54.44 -17 50 32.8 27.22049 19 23 49.28 -17 55 08.2 The following parabolic orbital elements have been determined by the undersigned. It is rather probable that the comet is a short-period one, and the ephemeris is uncertain by perhaps 1o. T = 1978 Jan. 23.28 ET Peri. = 61.11 Node = 146.22 1950.0 q = 2.2828 AU Incl. = 5.72 1979 ET R. A. (1950) Decl. Delta r m1 Aug. 15 19 15.73 -18 34.9 3.513 4.394 19.2 25 19 13.26 -18 52.8 Sept. 4 19 12.25 -19 07.9 3.882 4.555 19.5 14 19 12.71 -19 19.9 24 19 14.56 -19 28.7 4.315 4.716 19.9 1979 August 29 (3397) Brian G. Marsden
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