Circular No. 4583 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 MARSDEN or GREEN@CFA.BITNET MARSDEN or GREEN@CFAPS2.SPAN TRANSIENT X-RAY SOURCE F. Makino and the Ginga Team, Sagamihara, Kanagawa, report: "Ginga discovered a new transient source on Apr. 3 at R.A. = 18h40m +/- 1m, Decl. = +0.8 +/- 0.1 deg (equinox 1950.0). The intensity was about 50 mCrab and was at the same level during monitoring on Apr. 10 and 19. The x-ray spectrum is hard and resembles that of an x-ray binary pulsar. Coherent pulsation search is underway." COMET LEVY (1988e) Improved parabolic orbital elements from MPC 13041: T = 1987 Nov. 29.870 ET Peri. = 326.864 Node = 288.138 1950.0 q = 1.18187 AU Incl. = 62.821 1988 ET R.A. (1950) Decl. Delta r m1 Apr. 19 22 09.07 +30 37.4 29 22 18.50 +35 03.6 2.851 2.479 12.7 May 9 22 26.37 +39 23.1 19 22 32.42 +43 34.6 2.920 2.702 13.1 29 22 36.29 +47 35.9 June 8 22 37.57 +51 24.5 2.994 2.922 13.5 18 22 35.72 +54 57.3 28 22 30.18 +58 09.9 3.076 3.141 13.9 July 8 22 20.47 +60 57.4 18 22 06.37 +63 14.1 3.174 3.356 14.3 Total visual magnitude estimates by D. Levy, Tucson, AZ: Apr. 9.46 UT, 12.3 (Catalina 1.54-m reflector); 19.47, 12.6 (0.4-m reflector); 20.46, 12.7 (0.4-m reflector). COMET LILLER (1988a) Further total visual magnitude estimates: Apr. 14.81 UT, 5.0 (M. V. Zanotta, Milan, Italy, 10 x 50 binoculars; tail 1 deg in p.a. 340 deg); 17.04, 5.9 (G. R. Chester, Rixeyville, VA, 7 x 50 binoculars; tail 1 deg in p.a. 350 deg); 18.46, 5.7 (A. Hale, Las Cruces, NM, 10 x 50 binoculars; 40' tail in p.a. 350 deg); 18.82, 5.0 (Zanotta, 1 deg tail in p.a. 355 deg); 21.47, 4.7 (Levy, 0.15-m reflector; 3 deg tail in p.a. about 20 deg); 22.04, 5.5 (D. W. E. Green, Cambridge, MA, 20 x 80 binoculars). 1988 April 22 (4583) Brian G. Marsden
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