Read IAUC 3773
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
Read IAUC 3773
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