Circular No. 3546 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 PROBABLE NOVA IN CYGNUS H. Kosai, Tokyo Astronomical Observatory, telexes that Minoru Honda, Kurashiki, has discovered a probable nova as follows: 1980 UT R. A. (1950) Decl. mv Nov. 29.41841 21 40.7 +31 15 10 The object is slowly increasing in brightness. UX URSAE MAJORIS R. J. Panek, A. V. Holm and F. H. Schiffer III, Computer Sciences Corporation and Goddard Space Flight Center, report: "IUE spectra of UX UMa on Nov. 25 show that the ultraviolet line emission reported on IAUC 3538 is still present but has weakened considerably since Oct. 15. Si IV is no longer detectable in the out-of-eclipse spectra. Optical spectrophotometry is urged." COMET MEIER (1980q) D. Bockelee-Morvan, J. Crovisier, E. Gerard and I. Kazes, Meudon Observatory and Nancay Radio Observatory, communicate: "The main lines of OH at 1667 and 1665 MHz were detected in absorption in comet 1980q on Nov. 16, 27 and 28 with the Nancay radio telescope. The 1667-MHz antenna temperature was -30 +/- 13 and -18 +/- 6 mK on Nov. 16 and on Nov. 27-28, respectively. The corresponding OH-parent production rates (reduced to 1 AU assuming an inverse-square-law dependence) are (9 +/- 3) x 10**28 and (15 +/- 4) x 10**28 molecules per second." Total visual magnitude estimates: Nov. 10.79 UT, 9.1 (G. S. Keitch, Wrington, Eng., 0.3-m reflector); 13.02, 10.5 (J. DeYoung, Palmyra, VA, 0.15-m reflector); 30.93, 9.5 (C. S. Morris, Harvard, MA, 0.25-m reflector). SU TAURI The following visual magnitude estimates of this R CrB-type variable (cf. IAUC 3524) have been reported by C. E. Spratt, Victoria, B.C.: Nov. 1.2 UT, 11.7; 8.2, 11.1; 10.3, 11.2; 14.3, 10.9. 1980 December 3 (3546) Brian G. Marsden
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