Circular No. 3716 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 COMET AUSTIN (1982g) The following precise positions have been measured by P. M. Kilmartin from exposures by A. C. Gilmore at Mt. John Observatory: 1982 UT R. A. (1950) Decl. July 2.70985 4 24 50.27 -36 52 00.3 2.71731 4 24 50.97 -36 51 53.6 6.77205 4 31 51.09 -35 44 03.8 6.78490 4 31 52.55 -35 43 49.8 15.64606 4 50 54.31 -32 26 51.4 15.66396 4 50 57.18 -32 26 21.3 Improved parabolic orbital elements determined by the undersigned from 17 observations June 19-July 15: T = 1982 Aug. 24.7259 ET Peri. = 33.8178 Node = 325.5726 1950.0 q = 0.647757 AU Incl. = 84.4954 These elements yield the following corrections to the ephemeris on IAUC 3708-3709: 1982 ET dR.A. dDecl. 1982 ET dR.A. dDecl. July 25 -0.36 - 5.3 Aug. 14 -2.47 -29.4 30 -0.67 -11.1 19 -2.09 -14.1 Aug. 4 -1.21 -22.4 24 -1.36 - 6.0 9 -1.98 -35.3 29 -0.80 - 3.1 TT ARIETIS J. Mattei, AAVSO, informs us that this object (cf. IAUC 3683) is again at minimum: according to J. Bortle, Stormville, NY, it was fainter than mv 14.7 on July 21.34 UT. RS OPHIUCHI Several observers have reported that this recurrent nova is unusually bright (the brightest since 1976). Selected visual magnitude estimates: June 22.16 UT, 11.7 (M. Heifner, Denver, CO; communicated by Mattei); 26.16, 11.4 (Heifner); 29.16, 10.7 (Heifner); July 4.9, 10.5 (M. Verdenet, Bourbon-Lancy, France); 8.9, 10.0 (Verdenet); 15.03, 10.3 (G. M. Hurst, Wellingborough, England); 19.98, 10.3 (Hurst); 20.14, 10.1 (Heifner); 21.14, 10.2 (Heifner). 1982 July 22 (3716) Brian G. Marsden
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