Circular No. 4018 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 617-495-7244/7440/7444 TT ARIETIS K. Beuermann and H. Weissieker, Technische Universitat, Berlin, telex: "Photometry with the 1-m telescope at the European Southern Observatory on Oct. 23.2 gave V = 13.22, B-V = +0.02, U-B = -1.18. CCD spectroscopy with the 3.6-m telescope on Oct. 23.2 and 24.2 showed intense Balmer emission lines with equivalent widths of ~ 5 nm for H-alpha, H-beta and H-gamma and weaker emissions of He I, He II and the 465-nm blend. The wings of the Balmer lines now extend to +/- 3500 km/s, suggesting that the accretion disk is building up again but has not yet reached the former optically thick state." Visual magnitude estimates: Nov. 11.74 UT, 14.0 (M. Verdenet, Bourbon-Lancy, France); 15.06, 13.6 (J. Bortle, Stormville, NY); 20.06, 13.8 (Bortle); 24.77, 14.9 (Verdenet); 28.01, 14.8 (Bortle). COMET LEVY-RUDENKO (1984t) Ephemeris continuation from the orbital elements on MPC 9293: 1984/85 ET R.A. (1950.0) Decl. p r m1 Dec. 6 18 38.80 +21 24.9 1.137 0.930 9.0 11 18 36.28 +24 07.7 16 18 33.40 +26 53.3 1.091 0.919 8.8 21 18 30.12 +29 43.8 26 18 26.33 +32 42.2 1.018 0.942 8.8 31 18 21.91 +35 52.4 Jan. 5 18 16.61 +39 19.7 0.925 0.997 8.8 10 18 10.02 +43 10.6 15 18 01.38 +47 32.8 0.821 1.077 8.9 20 17 49.25 +52 34.3 25 17 30.64 +58 20.5 0.720 1.174 9.0 30 16 58.85 +64 46.0 Feb. 4 15 57.4 +71 12.9 0.648 1.285 9.1 9 13 55.5 +75 27.9 14 11 22.0 +73 48.8 0.635 1.402 9.5 19 9 48.86 +67 16.5 24 9 03.97 +59 23.7 0.702 1.525 10.1 Mar. 1 8 40.85 +51 50.5 6 8 28.07 +45 10.5 0.841 1.650 10.8 11 8 20.86 +39 29.7 16 8 16.97 +34 43.4 1.032 1.777 11.6 1984 December 10 (4018) Brian G. Marsden
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