Circular No. 3998 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 COMET SHOEMAKER (1984q) Further positions have been reported as follows: 1984 UT R.A. (1950.0) Decl. Observer Oct. 4.1695 23 06.85 +18 13.2 Gibson 5.17049 23 05 44.36 +18 22 59.3 Tatum J. Gibson (Palomar). 1.2-m Schmidt. J. B. Tatum (University of Victoria). 0.25-m f/2 Schmidt. The following parabolic orbital elements are based on the three accurate positions. The comet may be a short-period one. T = 1984 June 30.87 ET Peri. = 343.36 Node = 345.06 1950.0 q = 2.1959 AU Incl. = 39.75 1984 ET R.A. (1950.0) Decl. p r m1 Oct. 2 23 09.36 +17 51.9 7 23 03.78 +18 39.7 1.546 2.468 12.9 12 22 58.99 +19 21.1 17 22 55.02 +19 56.9 1.661 2.522 13.1 22 22 51.91 +20 28.2 27 22 49.67 +20 56.0 1.797 2.578 13.4 NOVA SAGITTARII 1984 W. Liller, Vina del Mar, Chile, provides the following revised and new approximate visual magnitude estimates: Sept. 25.02 UT, 10.3; 25.99, 9.7; 27.00, 10.5; 29.01, 10.6; Oct. 3.02, 10.6. H. Pedersen, La Silla, reports that M. P. and P. Veron observed the nova over the range 610-710 nm using the 2.2-m European Southern Observatory telescope with the Boller and Chivens spectrograph and CCD detector. Broad, asymmetric H-alpha emission was present on Oct. 4 with a width of 6.8 nm (3100 km/s) at the base. NSV 2229 This object (cf. IAUC 3924, etc.) was not recorded down to mag ~ 13 photographically on Sept. 6 by D. di Cicco, Sudbury, MA; and to mag ~ 15 visually on Sept. 22 by di Cicco and also by M. Verdenet, Bourbon-Lancy, France. 1984 October 5 (3998) Brian G. Marsden
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