Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 4382: 1987E; 1987A; T Leo; 1987B

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 4381  SEARCH Read IAUC 4383
IAUC number


                                                  Circular No. 4382
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 617-495-7244/7440/7444


SUPERNOVA 1987E IN NGC 4725?
     P. Wild, Astronomical Institute, University of Berne, reports
the existence of a foreground star, with a proper motion of 0".13/yr
in p.a. 285 deg, at the given position of this object (IAUC 4373); he
detects no unusual brightening in this object (mag about 16).


SUPERNOVA 1987A IN THE LARGE MAGELLANIC CLOUD
     M. Karovska, P. Nisenson, R. Noyes, and C. Papaliolios, Center
for Astrophysics, write:  "High-angular-resolution speckle observations
of SN 1987A on Mar. 25 and Apr. 2 using the Cerro Tololo
Interamerican Observatory 4-m telescope (with the CfA PAPA photon-
counting detector) show a bright feature with a separation of 0".057
+/- 0".014 at p.a. 194 deg +/- 5 deg relative to the SN.  This feature appears
to be 2.7 +/- 0.2 mag fainter than the SN in a 10-nm bandpass centered
on 656.3 nm (H-alpha).  A corresponding feature was detected in a
10-nm bandpass centered at 533 nm, though it appears to be somewhat
fainter than in H-alpha.  Preliminary analysis of data recorded in a 10-
nm bandpass centered at 450 nm shows no evidence of an object
within a 4-mag difference from the SN.  Data from nearby comparison
stars, recorded close in time using the same filters, produced
clean, point-like images with no structure above the noise at the
separation and position angle of the observed feature."
     Corrigendum.  On IAUC 4370, lines 7-15, for  mm  read  microns
     Visual magnitude estimates:  Apr. 28.51 UT, 3.0 (R. McNaught,
Siding Spring Observatory); 29.38, 3.0 (D. A. J. Seargent, The
Entrance, N.S.W.); 30.43, 2.9 (McNaught).


T LEONIS
     This star has had another outburst, as shown by the following
visual magnitude estimates (reported via G. M. Hurst, Basingstoke,
England, and J. Mattei, AAVSO):  Apr. 28.89 UT, [13.7: (S. Lubbock,
Bridgend, Wales); May 1.12, 10.5 (G. Dyck, N. Dartmouth, MA); 1.90,
11.2 (Lubbock); 2.08, 11.8 (P. Dombrowski, Glastonbury, CT).


SUPERNOVA 1987B IN NGC 5850
     Corrigendum: On IAUC 4370, the three observations by J. Griese
are to be deleted.


1987 May 4                     (4382)            Daniel W. E. Green

Read IAUC 4381  SEARCH Read IAUC 4383


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


Valid HTML 4.01!