Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 4925: 1989e1; NGC 7078; 1989r

The following International Astronomical Union Circular may be linked-to from your own Web pages, but must not otherwise be redistributed (see these notes on the conditions under which circulars are made available on our WWW site).


Read IAUC 4924  SEARCH Read IAUC 4926
IAUC number


                                               Circular No. 4925
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 or GREEN@CFA.BITNET    MARSDEN or GREEN@CFAPS2.SPAN


COMET GEORGE (1989e1)
     Douglas B. George, Kanata, near Ottawa, reports his visual
discovery of a comet.  The following observations are available:

     1989 UT           R.A. (1950) Decl.        m1       Observer
     Dec. 18.031      19 52.3      +25 30      13        George
          19.073      19 54.2      +25 35      10.5      Hale
          19.115      19 54.4      +25 32      10.4      Levy

D. B. George (Kanata, ON).  0.40-m reflector.
A. Hale (Las Cruces, NM).  0.41-m reflector.  Object diffuse with
  central brightening.
D. Levy (Tucson, AZ).  0.41-m reflector.  Comet diffuse with slight
  condensation and 2' coma; faint sunward fan at p.a. 240 deg.


NGC 7078
     H. Lehto, G. Machin, I. McHardy, and P. Callanan, Department
of Astrophysics, University of Oxford; and P. Charles, Royal
Greenwich Observatory, report:  "We have made Very Large Array
observations at 6 cm in 1989 Feb. of the globular cluster NGC 7078
(M15).  A deep map (rms 28 mJy) revealed the presence of a 185-mJy
source in the core of the cluster at a position of R.A.
= 21h27m33s.28, Decl. = +11 56'50".9 (equinox 1950.0) with an
uncertainty of +/- 0".4.  The coincidence of this position with AC
211, the optical counterpart of the x-ray source (Geffert et al.
1989, A.Ap. 209, 423), implies that the x-ray system is the source
of the emission.  There is evidence that the emission region is
extended."


COMET OKAZAKI-LEVY-RUDENKO (1989r)
     Total visual magnitude estimates (cf. IAUC 4918):  Dec. 6.49
UT, 6.5 (G. W. Wolf, Wellington, N.Z., 20x50 binoculars); 7.68, 6.4
(G. Garradd, Tamworth, N.S.W., 10x50 binoculars); 8.81, 6.5 (A.
Pearce, Scarborough, W. Australia, 20x80 binoculars); 10.60, 6.6
(D. A. J. Seargent, The Entrance, N.S.W., 15x80 binoculars); 11.38,
7.0 (Wolf, 0.06-m refractor; 12' tail in p.a. 300o); 11.83, 7.4
(Pearce); 15.45, 7.7 (Garradd); 17.48, 7.2 (Seargent); 18.48, 6.9
(Seargent).


1989 December 19               (4925)             Daniel W. E. Green

Read IAUC 4924  SEARCH Read IAUC 4926


Our Web policy. Index to the CBAT/MPC/ICQ pages.


Valid HTML 4.01!