Circular No. 5164 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Telephone 617-495-7244/7440/7444 (for emergency use only) TWX 710-320-6842 ASTROGRAM CAM EASYLINK 62794505 MARSDEN or GREEN@CFA.BITNET MARSDEN or GREEN@CFAPS2.SPAN PERIODIC COMET SWIFT-GEHRELS (1991c) S. Nakano, Sumoto, Japan, reports the recovery of this comet by T. Seki, Geisei, as given below. The comet is diffuse with central condensation. The indicated correction to the prediction on MPC 13045 (ephemeris on MPC 16449) is Delta(T) = +0.06 day. 1991 UT R.A. (1950) Decl. m1 Jan. 7.39167 22 12 00.12 - 5 30 29.5 16.5 7.41500 22 12 03.56 - 5 30 02.4 12.40747 22 25 42.59 - 3 59 01.4 17.0 13.38924 22 28 26.18 - 3 40 44.4 17.0 13.39896 22 28 27.58 - 3 40 30.7 13.41042 22 28 29.68 - 3 40 17.5 13.42326 22 28 31.79 - 3 40 02.5 SUPERNOVA 1991B IN NGC 5426 M. M. Phillips, Cerro Tololo Interamerican Observatory, reports that a spectrogram of SN 1991B obtained by Mario Hamuy with the CTIO 1.5-m telescope on Jan. 15.35 UT shows that this is a type-Ia supernova about 20 days past B maximum. HD 50138 Y. Andrillat and L. Houziaux, Observatoire de Haute-Provence, "This B[e] object (HD 50138 = MWC 158) seems to have undergone an important new shell phase. On CCD spectrograms (range 757-955 nm, resolution 0.13 nm) obtained at Haute-Provence Observatory, line features differ markedly from 1990 January observations. The double symmetrical O I emission at 777.3 nm shows, on 1990 Dec. 29, an inverted P-Cyg profile with emission of 1.11 and a deep absorption of 0.76 in terms of the local continuum with m(777) = 8.11. Double emission Paschen lines from P9 to P22 indicate a red-shifted absorption, while the V/R ratios present important changes. O I 844.6-nm emission peaks at twice the local continuum, m(845) = 7.52, while the 926.5-nm line is absent." 1991 January 15 (5164) Daniel W. E. Green
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