Circular No. 5350 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Telephone 617-495-7244/7440/7444 (for emergency use only) TWX 710-320-6842 ASTROGRAM CAM EASYLINK 62794505 MARSDEN or GREEN@CFA.BITNET MARSDEN or GREEN@CFAPS2.SPAN 1991 RC Further precise positions have been reported as follows: 1991 UT R.A. (1950) Decl. V Observer Sept.13.54492 21 57 13.22 -11 12 27.5 18.5 Hartley 17.19326 21 49 19.90 -12 28 05.2 Scotti 17.20201 21 49 18.81 -12 28 15.2 " 17.21062 21 49 17.70 -12 28 25.0 " M. Hartley (Siding Spring). 1.2-m U.K. Schmidt. Beginning of faint trail. Measurer R. H. McNaught. J. V. Scotti (Kitt Peak). 0.91-m Spacewatch telescope. Improved elements, from the eight observations Sept. 3-17, show that the orbit is very similar to that of (1566) Icarus: T = 1991 Apr. 23.613 ET Peri. = 8.161 e = 0.82871 Node = 160.645 1950.0 q = 0.18536 AU Incl. = 23.543 a = 1.08214 AU n = 0.875551 P = 1.13 years 1991 ET R.A. (1950) Decl. Delta r V Sept.11 22 03.27 -10 14.7 0.859 1.843 18.6 16 21 51.81 -12 04.2 21 21 42.09 -13 37.5 0.962 1.882 19.2 26 21 34.14 -14 55.3 Oct. 1 21 27.88 -15 59.1 1.090 1.914 19.7 6 21 23.21 -16 50.3 11 21 19.99 -17 30.6 1.234 1.940 20.1 AM HERCULIS H. Jessop, Sonoma State University; and P. A. Mason, Louisiana State University, report that AM Her remains in its low accretion state (cf. IAUC 5312). Cooled CCD observations made with the Sonoma State University 0.17-m telescope indicate that AM Her was at V = 15.1 (orbital average) and that it did not vary from this average by more than 0.2 mag during 3.2 hr of 1-min integrations. The observations were centered on Sept. 5.24 UT, and the result is consistent with low- state behavior. 1991 September 18 (5350) Brian G. Marsden
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