Circular No. 4478 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 1987 UA Another fast-moving asteroidal object has been discovered by C. Shoemaker on films taken with the 0.46-m Schmidt telescope at Palomar by E. Shoemaker and H. Holt, with the following measurements by C. Shoemaker available: 1987 UT R. A. (1950) Decl. Mag. Oct. 17.32483 0 22 55.50 - 0 45 41.5 16.5 19.38073 0 27 18.12 - 2 56 11.4 21.20981 0 31 13.40 - 4 46 07.8 The following orbital elements by C. M. Bardwell, Center for Astrophysics, from the above observations suggest that this is an Amor-type object: T = 1987 Oct. 6.97 ET Peri. = 173.36 e = 0.2873 Node = 197.64 1950.0 a = 1.7007 AU i = 16.09 n = 0.44438 q = 1.2121 AU P = 2.22 years 1987 ET R.A. (1950) Decl. Delta r V Oct. 22 0 32.88 - 5 31.3 0.239 1.219 16.2 27 0 43.37 - 9 50.3 Nov. 1 0 53.65 -13 17.3 0.276 1.230 16.7 6 1 03.68 -15 54.6 11 1 13.42 -17 47.3 0.326 1.246 17.3 16 1 22.90 -19 01.6 21 1 32.16 -19 43.2 0.385 1.268 17.8 26 1 41.27 -19 57.5 Dec. 1 1 50.28 -19 49.4 0.450 1.293 18.2 GX 9+9 B. E. Schaefer, Goddard Space Flight Center, writes: "The optical counterpart of the x-ray binary GX 9+9 is found to have a sinusoidal modulation with amplitude 0.5 mag and period 4.198 +/- 0.008 hr. The 212 individual observations were obtained during June 16-27 with the 0.9-m telescope (+ CCD camera and B filter) at Cerro Tololo Interamerican Observatory. This period is consistent with the x-ray period reported by Hertz and Wood (IAUC 4221)." 1987 October 26 (4478) Daniel W. E. Green
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