Circular No. 4001 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 PERIODIC COMET KOWAL-MRKOS (1984n) A. Mrkos, Klet Observatory, provides additional observations: 1984 UT R.A. (1950.0) Decl. m1 May 19.91340 13 06 58.68 -10 04 20.6 16.0 19.92752 13 06 58.95 -10 04 18.2 Improved orbital elements from 8 observations Apr. 23-May 19: T = 1984 June 7.6307 ET Peri. = 338.1046 e = 0.482556 Node = 248.4996 1950.0 a = 3.770605 AU Incl. = 2.9568 n = 0.1346132 q = 1.951075 AU P = 7.322 years 1984 ET R.A. (1950.0) Decl. p r m1 Oct. 7 16 45.91 -21 10.0 2.534 2.199 18.4 17 17 07.86 -21 37.8 27 17 29.86 -21 54.7 2.789 2.277 18.8 Nov. 6 17 51.80 -22 00.6 16 18 13.56 -21 55.3 3.033 2.360 19.1 26 18 35.04 -21 39.1 Dec. 6 18 56.16 -21 12.6 3.257 2.449 19.5 2S 0142+61 The following remarks should have been included in the item by White et al. on IAUC 3996: "The EXOSAT CMA 10" error circle is centered at R.A. = 1h42m52s9, Decl. = +61deg29'49" (equinox 1950.0), and overlaps the Einstein HRI position (obtained from the Einstein data base) of R.A. = 1h42m53s7, Decl. = +61deg30'05". F. Seward notes that the 90-percent-confidence random uncertainty in the Einstein position is 3", but this particular position may have an additional systematic offset of 5". Using the star numbering convention of Reid et al. (1980, A.J. 85, 1062), we note that star 3 lies 10" and 18", and that star 8 lies 8" and 12", respectively, from the centers of the EXOSAT and Einstein HRI error circles." SUPERNOVA IN NGC 991 Visual magnitude estimates by R. McNaught, Coonabarabran, NSW: Sept. 3.67 UT, 14.1; 6.80, 14.4; 22.69, 15.0; Oct. 15.55, 15.8. 1984 October 25 (4001) Brian G. Marsden
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