Circular No. 4224 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 SUPERNOVA 1986G IN NGC 5128 V. M. Blanco, Cerro Tololo Interamerican Observatory, reports the following photometric measurements, obtained on May 11.09 UT: V = 11.46, B-V = +1.02, V-B = +0.78, V-I (Cousins) = +0.85. J. Aycock, F. Baas, M. F. Bode, T. R. Geballe, A. J. Longmore, A. D. MacFadzean, M. G. Smith and D. M. Walther, in collaboration with J. R. Graham and W. P. S. Meikle, report: "A 7-channel cooled grating spectrometer, mounted on the U.K. Infrared Telescope, Mauna Kea, was used to measure spectra in the J, H and K windows on May 24, 25 and 26, respectively. The spectra show many prominent, broad, absorption/emission features in each band, to an extent that makes the continuum difficult to define. Of particular note is a very broad and deep 'absorption' that appears to extend from 1.20 to 1.55 microns (FWHM). However, at present our spectra do not cover the region from 1.36 to 1.49 microns, so the intensity could peak again in the unobserved spectral region. The short-wavelength end of this remarkable feature is clearly responsible for the extremely red J-H colors of classical type I supernovae at this epoch. At first sight the explanation of the red J-H colors as due to absorption by Si I 1.203 micron (Graham 1986, M.N.R.A.S. 220, 27P) seems unlikely because the wavelength of the absorption should be blueshifted by ~ 10 000 km/s and consequently should occur at 1.16 microns." Visual magnitude estimates by R. O. Evans (E), Hazelbrook, and R. H. McNaught (M), Coonabarabran, N.S.W., the first six correcting those on IAUC 4208: May 3.5 UT, 12.0 (E); 3.545, 11.8 (M); 3.589, 11.9 (M); 4.5, 12.5 (E); 4.507, 12.4 (M); 4.654, 11.8 (M); 6.6, 11.8 (E); 7.35, 12.3 (E); 8.5, 12.0 (E); 9.5, 12.0 (E); 10.5, 11.9 (E); 11.5, 11.6 (E); 12.4, 11.6 (E); 13.63, 11.8 (M); 14.53, 11.7 (M); 15.38, 11.6 (M); 16.39, 11.8 (M); 18.61, 11.8 (M); 20.65, 11.9 (M); 21.49, 12.2 (M); 28.48, 12.7 (M); 29.46, 12.9 (M); 30.47, 12.8 (M); 31.41, 13.3 (M); June 1.51, 13.5 (M). KUWANO'S OBJECT IN AQUILA = CGSS 1175 M. Morel, Rankin Park, N.S.W., notes that this object appears to be identical with star 1175 of Stephenson's (1984, Publ. Warner Swasey Obs. 3, No. 1) "General Catalogue of Galactic S Stars" (2nd edition), where its magnitude is given as mv = 10.5 and its spectrum as M6S. Further visual magnitude estimates by McNaught: May 25.6 UT, 9.5; 28.63, 9.7. 1986 June 3 (4224) Brian G. Marsden
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