Circular No. 3255 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 617-864-5758 SUPERNOVA IN MCG -5-9-22 V. M. Blanco, Cerro Tololo Interainerican Observatory, further reports that F. Schweizer, M. M. Phillips and J. H. Elias have analyzed a spectrogram of the supernova in MCG -5-9-22 obtained by A. C. Danks on Aug. 14.4 UT with the 400-cm telescope plus image-tube spectrograph and covering the wavelengths 4700-7000 A. The supernova is of type II with a featureless spectrum except for about 8000-km-s**-1-wide (fwhm) H-alpha and H-beta emission lines with P-Cyg profiles. The centers of the blue-shifted broad absorption components show expansion velocities of 7900 km s**-1 with respect to the galaxy, whose northern spiral arm has a heliocentric radial velocity of 4060 km s**-1 For a Hubble constant of 50 km s**-1 Mpc**-1, the galaxy lies at a distance of about 80 Mpc, and the blue absolute magnitudes uncorrected for absorption are ~ -20.4 and -16.0 for the galaxy and supernova, respectively. Because of the scarcity of suitable published spectra of type II supernovae, the date of the light maximum cannot be estimated from this single spectrogram. The current absolute magnitude seems to be somewhat bright for a six-month-old supernova. Information from plates of the galaxy taken since January would be most useful to establish or refute the proposed identification with the x-ray burst of Feb. 2 (IAUC 3254). 1978 PA H.-E. Schuster, European Southern Observatory, communicates the following additional semiaccurate positions: 1978 UT R. A. (1950) Decl. Aug. 14.25139 0 08 07 -41 04.6 15.29028 0 08 30 -41 34.0 1978 P 1 J. D. Mulholland, University of Texas at Austin, reports that a 10-min exposure of Pluto was obtained by P. J. Shelus on 1977 May 22.23 UT with the 208-cm reflector at the McDonald Observatory. The plate scale was ~ 7".5/mm and the seeing 1" or better. The image of Pluto was elongated by 10-15 percent in p.a. 180o+ 10o, in good agreement with the prediction (IAUC 3241). A nearby star was elongated by no more than about 1 percent. 1978 August 16 (3255) Daniel W. E. Green
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