Circular No. 3772 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 lambda ANDROMEDAE S. L. Baliunas, A. K. Dupree and E. F. Guinan, Center for Astrophysics, report that a large increase in the ultraviolet emission-line fluxes of the long-period RS-CVn giant lambda And was observed with IUE during the photometric minimum of the 54-day rotation period. The maximum of the flare occurred at about 1982 Nov. 6.31 UT with the emission-line fluxes of C III 118 nm, C IV 155 nm and Ly-alpha 122 nm showing the greatest enhancements of ~ 3 to 5 times relative to their quiescent values. The risetime of the flare was ~ 60 to 90 min, while the decay time was > 5 hr. This appears to be the first time a flare event of this kind has been observed for a cool giant star, and it is suggested that the star be monitored more intensively at all wavelengths during 1983 Feb. 23-28, the next predicted light minimum. PERIODIC COMET CHURYUMOV-GERASIMENKO (1982f) Further total visual magnitude estimates: Feb. 1.81 UT, 10.4 (J.-C. Merlin, Le Creusot, France, 0.26-m refl.); 4.83, 10.6 (Merlin); 11.04, 10.6 (J. Bortle, Stormville, NY, 0.32-m refl.). Ephemeris continuation from the elements on IAUC 3743: 1983 ET R.A. (1950.0) Decl. p r m1 Feb. 15 7 19.46 +36 44.3 0.826 1.699 13.0 25 7 28.49 +35 16.6 Mar. 7 7 39.53 +33 45.9 1.084 1.839 14.1 17 7 52.06 +32 13.9 27 8 05.68 +30 41.3 1.390 1.985 15.2 Apr. 6 8 20.01 +29 08.2 16 8 34.77 +27 34.4 1.732 2.133 16.1 26 8 49.80 +25 59.8 May 6 9 04.90 +24 24.4 2.098 2.281 17.0 16 9 19.99 +22 48.1 26 9 34.99 +21 10.9 2.474 2.428 17.7 SU TAURI Visual magnitude estimates by J. Bortle, Stormville, NY: Jan. 22.0 UT, 12.2; Feb. 2.0, 11.5; 10.1, 10.8; 11.1, 11.0. 1983 February 14 (3772) Brian G. Marsden
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