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Circular No. 5933
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@CFA or GREEN@CFA (.SPAN, .BITNET or .HARVARD.EDU)
PERIODIC COMET WILD 3 (1994b)
J. V. Scotti and T. Gehrels, Lunar and Planetary Laboratory,
report that they have recovered this comet with the 0.9-m Spacewatch
Telescope at Kitt Peak, as shown below. On Feb. 10, there was a
coma 12" across and tail 0'.29 long in p.a. 292 deg (m2 = 22.3).
The indicated correction to the prediction on MPC 18258 (ephemeris
on MPC 23139) is Delta(T) = +0.03 day.
1994 UT R.A. (2000) Decl. m1
Feb. 10.49233 15 11 48.72 - 4 00 10.9
10.49730 15 11 48.96 - 4 00 12.0 20.7
10.50515 15 11 49.55 - 4 00 12.7 21.2
10.51078 15 11 49.78 - 4 00 13.7
10.51564 15 11 50.14 - 4 00 15.0
13.50508 15 14 53.30 - 4 09 03.6
13.51935 15 14 54.25 - 4 09 04.7
A0535+26
R. B. Wilson and B. A. Harmon, Marshall Space Flight Center,
NASA; and M. H. Finger, Computer Sciences Corporation, report for
the Compton Gamma Ray Observatory BATSE team: "The outburst
reported on IAUC 5931 has continued and intensified through Feb. 8.
The daily phase-averaged pulsed intensity in the band 20-40 keV,
relative to the total Crab Nebula flux (pulsed + steady), was 0.2,
0.5, 0.7, 0.8, 0.9, and 1.1 on Feb. 3-8. The daily total intensity
(also 20-40 keV), measured using Earth occultation, was 0.4, 0.9,
1.4, 1.9, 2.2, and 2.7 relative to the total Crab Nebula flux. All
values stated above are accurate to +/- 5 percent. The source is
detectable to at least 100 keV."
SU TAURI
B. S. Carter, South African Astronomical Observatory, reports:
"Observation of SU Tau by F. Marang on Jan. 29.89 using the 0.75-m
telescope yields magnitudes J = 11.74, H = 9.22, K = 7.14, L =
4.59, which indicates that a dust shell has been ejected."
1994 February 14 (5933) Daniel W. E. Green
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