Circular No. 3127 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Cable Address: SATELLITES, NEWYORK Telex: 921428 Telephone: (617) 864-5758 COMET SANGUIN (1977p) R. M. West, European Southern Observatory, provides the following precise positions, measured from plates taken by H.-E. Schuster: 1977 UT R. A. (1950) Decl. Oct. 20.24347 22 34 18.37 - 8 20 49.0 21.00908 22 35 15.40 - 8 29 36.1 COMET KOHLER (1977m) D. Despois, E. Gerard, B. Darchy and J. Pezzani report that observations with a dual linear-polarization 50-K receiver at Nancay Radio Observatory since Oct. 21 show the OH line at 1667 MHz in absorption; the brightness temperature is about -0.13 K and the line width 3 km/s. The OH gas production is comparable to that of comet Kohoutek (1973 XII). The brightness temperature is increasing owing to the approaching background galactic ridge and should reach ~ -4 K during Nov. 2-5. SMC X-2 AND SMC X-3 P. Pesch, Warner and Swasey Observatory, communicates: "On a deep, nitrogen-baked, objective-prism plate taken with the Curtis Schmidt telescope at Cerro Tololo Interamerican Observatory, N. Sanduleak and A. G. D. Philip note the presence of a fourteenth-magnitude OB star within ~ 0'.5 of the position given for SMC X-2 (IAUC 3125). The star can be identified in Fig. 1 of Sanduleak 1968, Astron. J. 73, 246), where it lies 23.9 mm almost due east of star No. 30 and 32.8 mm from star No. 60. About 20" due west of the OB star there is a pair of slightly fainter stars lying along a northeast-southwest axis. Corrigendum. On IAUC 3125, the value of R.A. for SMC X-3 should read 0h50m21s.2, not 0h52m21s.2 NOVA SAGITTARII 1977 Further visual magnitude estimates: Aug. 16.10 UT, 11.4 (5. O'Meara, Harvard Observatory); 26.11, 11.4 (O'Meara); Sept. 7.13, 11.7 (J. Bortle, Brooks Observatory); 20.5, 11.3 (V. L. Matchett, Indooroopilly, Queensland); Oct. 22.1, 11.8 (Bortle). 1977 October 31 (3127) Brian G. Marsden
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