Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 4417: 1987I; 1987A; 1987l; 1987m

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 4416  SEARCH Read IAUC 4418
IAUC number


                                                  Circular No. 4417
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 1987I IN IC 4963
     D. Allen, Anglo-Australian Observatory, reports his discovery
of a supernova located 1".6 north and 1".5 east of the center of IC
4963 (R.A. = 20h08m11s, Decl. = -55 23.7, equinox 1950.0).  A low-
dispersion spectrum of the galaxy, obtained under poor conditions with
the Mt. Stromlo 1.9-m telescope on July 2.71 UT, is dominated by
features typical of a type-I SN.  Observations by K. Cooper on
July 2 with the Anglo-Australian Telescope show a redshift of 0.017
as deduced from both H-alpha emission in the galaxy and the 615-nm
absorption band in the SN; the magnitude is about 16.


SUPERNOVA 1987A IN THE LARGE MAGELLANIC CLOUD
     C. Perrier, Observatoire de Lyon, telexes:  "Infrared speckle
observations of SN 1987A were performed in June using the scanning
slit specklegraph at the European Southern Observatory 3.6-m telescope.
The observations (in 2".0 seeing or better at V and obtained
near the meridian) were made mostly at L (3.6 microns).  Various checks
were made with identical settings on binaries and pointlike sources
of similar magnitude.  Fits of the data from June 16 to 23 show
marginal evidence of a circularly-symmetric extension.  Attributing
50 percent of the supernova L flux to this component would yield a
FWHM of 0".057 +/- 0".030.  No significant departure from circular
symmetry (which could be due to the visible companion; cf. IAUC 4382,
4391) is detected, allowing derivation of a minimum magnitude
difference (companion vs. SN) of 4 +/- 1 at L.  Complementary measures
are needed to confirm the possible extension."
     Visual magnitude estimates:  July 4.75 UT, 4.4 (A. Beresford,
Adelaide, S. Australia); 6.82, 4.4 (R. H. McNaught, Siding Spring
Observatory); 7.36, 4.3 (Beresford); 8.83, 4.4 (McNaught).


PERIODIC COMET REINMUTH 2 (1987l)
     Total visual magnitude estimates:  July 6.25 UT, 14.3 (D. W.
E. Green, Oak Ridge Observatory, 0.41-m reflector); 8.40, 13.7 (D.
H. Levy, Tucson, AZ, 0.41-m reflector); 9.45, 13.8 (Levy).


PERIODIC COMET BROOKS 2 (1987m)
     Total visual magnitude estimates:  July 3.44 UT, 14.5: (J. V.
Scotti, Tucson, AZ, 0.4-m reflector); 4.41, 14.1 (Levy).


1987 July 9                    (4417)            Daniel W. E. Green

Read IAUC 4416  SEARCH Read IAUC 4418


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


Valid HTML 4.01!