Circular No. 4179 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 HALLEY (1982i) R. Gehrz, University of Minnesota, reports the following preliminary infrared magnitudes, obtained with the 2.3-m Wyoming Infrared Telescope: Jan. 11.9 UT (5"0 beam, 18" throw): [2.3 microns] = 7.56, [3.6 microns] = 5.02, [4.9 microns] = 2.80, [8.7 microns] = 0.72, [10.0 microns] = 1.24; N = 1.14, [11.4 microns] = 1.61, [12.6 microns] = 1.46, Q = 2.41, [23 microns] = 2.45; Jan. 12.9 (5"0 beam, 18" throw): 6.80, 4.18, 2.10, 1.06, 1.91, 1.49, 2.15, 2.12, 3.13, 3.48; Feb. 9.83 (8"3 beam, 18" throw): 4.33, 1.58, 0.28, 2.54, 3.84, 3.01, 3.71, 3.46, -, 4.55; Feb. 11.88 (8"3 beam, 20" throw): 3.80, 1.25, 0.54, 2.73, 3.94, 3.20, 3.63, 3.64, 4.56, 4.72. The 10-micron and 20-micron silicate emission features are present on all dates. W. E. Celnik, R. Schulz and K. Weissbauer, European Southern Observatory, report tail lengths on Feb. 18.4 UT of 34' in integrated light and 13' in CO+ (426 nm); the outer coma, of diameter 2'7, was limited in the solar direction by a bright, narrow, parabolic bow shock. On Feb. 19.4 the tail, more than 58' long in red light, was split into four narrow antisolar subtails and a broad unstructured antitail eastward; the outer coma was 4'3 in diameter, and the bow shock more intense than on Feb. 18; in CN (388 nm) the coma appeared diffuse and showed a short antisolar jet tail. H. Pedersen, B. Gelly and R. M. West report that the addition of four ESO wide-field CCD frames on Feb. 20.39 showed the following multiple tail structure: 1A, 100' long in p.a. 270, bifurcated at 70' from the head; 1B, 110' long in p.a. 275; 2, 90' in 280, strong and narrow; 3, 80' in 290, somewhat weaker and narrow; 4A, 90' in 315, bifurcated at 70'; 4B, 100' in 320, weaker; 5, 90' in 340, broad and diffuse; 6, > 70' in 3-30, very broad, masked by horizon; 7, 15' in 65, sharply defined edge. Total visual magnitude estimates: Feb. 15.13 UT, 3.8 (R. Fleet, Harare, Zimbabwe, 11 x 80 binoculars); 15.51, 3.5 (P. Maley, Houston, TX, 0.13-m refractor); 16.12, 3.6 (Fleet); 19.13, 2.8 (Fleet; tail 0.7 deg in p.a. 285P); 19.87, 3.5 (T. Seki, Geisei, Japan, 0.09-m refractor; tail 3 deg long); 20.56, 2.5 (J. Young, Table Mountain Observatory, 0.61-m reflector). SUPERNOVA 1986A IN NGC 3367 D. Herald, Canberra, has measured the following precise position from an exposure by P. Anderson, Brisbane: R.A. = 10h43m57s52, Decl. = +14deg00'49"7 (equinox 1950.0). 1986 February 20 (4179) Brian G. Marsden
Our Web policy. Index to the CBAT/MPC/ICQ pages.