Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 6282: X-RAY N 1992 IN SMC; C/1995 Q1

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 6281  SEARCH Read IAUC 6283

View IAUC 6282 in .dvi or .ps format.
IAUC number


                                                  Circular No. 6282
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Postal Address: Central Bureau for Astronomical Telegrams
Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions)
BMARSDEN@CFA.HARVARD.EDU or DGREEN@CFA.HARVARD.EDU (science)
Phone 617-495-7244/7440/7444 (for emergency use only)


X-RAY NOVA 1992 IN SMALL MAGELLANIC CLOUD
     G. Clark and R. Remillard, Massachusetts Institute of Technology;
and J. Woo, Harvard-Smithsonian Center for Astrophysics, report:
"A ROSAT observation of 1992 Oct. 1-2 discovered an x-ray nova located
5' southeast of SMC X-1 at R.A. = 1h17m41s.9, Decl. = -73d31'01"
(equinox 2000.0).  The object was not detected in a similar observation
359 days earlier, but it was detected 246 days later at a counting rate
diminished by a factor of 267, which corresponds to an average e-folding
decay time of 44 days.  The flux varied on a timescale of an hour or
less during the 1992 observation, but no periodic pulsations have been
detected.  The 1992 flux level would be produced by a source in the SMC
radiating isotropically with a luminosity in excess of 2.5 x 10**37
erg/s.  The 5"-radius positional error circle includes a blue star of
about mag 14 that should be an easy target for the optical measurements
required to determine whether it is the binary companion of a blackhole.
If it is, this nova will be the first blackhole x-ray nova with a massive
early-type companion."


COMET C/1995 Q1 (BRADFIELD)
     Continuation to the ephemeris on IAUC 6225 (elements MPC 26143):

1995/96     R. A. (2000) Decl.     Delta      r    Elong. Phase      m1
Dec. 29     2 09.22    +65 35.7    1.640    2.309  121.3   21.3     10.7
Jan.  8     1 55.61    +59 15.2    1.876    2.451  114.4   21.4     11.3
     18     1 52.96    +54 24.1    2.138    2.590  106.1   21.4     11.8
     28     1 55.35    +50 47.0    2.416    2.726   97.5   21.0     12.3
Feb.  7     2 00.43    +48 07.3    2.702    2.859   88.9   20.2     12.7
     17     2 07.10    +46 11.3    2.989    2.990   80.5   19.0     13.1
     27     2 14.77    +44 48.7    3.272    3.118   72.3   17.6     13.5
Mar.  8     2 23.06    +43 51.6    3.547    3.244   64.4   16.0     13.9
     18     2 31.76    +43 14.3    3.808    3.369   56.8   14.3     14.2
     28     2 40.69    +42 52.5    4.055    3.491   49.5   12.6     14.5
Apr.  7     2 49.70    +42 42.9    4.283    3.611   42.7   10.8     14.7
     17     2 58.71    +42 43.1    4.491    3.730   36.3    9.2     15.0
     27     3 07.60    +42 51.3    4.676    3.847   30.8    7.7     15.2

     Visual magnitudes: Nov. 16.12 UT, 9.6 (C. E. Spratt, Victoria, BC,
0.20-m refl.); 18.03, 9.4 (J. D. Shanklin, Cambridge, England, 14 x 100
binoculars); 18.31, 10.6 (A. Hale, Cloudcroft, NM, 0.41-m refl.); 20.12,
9.9 (Spratt); 30.49, 11.0 (Hale); Dec. 23.12, 10.1 (Spratt); 24.12, 10.5
(Spratt).

                      (C) Copyright 1996 CBAT
1996 January 2                 (6282)              Brian G. Marsden

Read IAUC 6281  SEARCH Read IAUC 6283

View IAUC 6282 in .dvi or .ps format.


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


Valid HTML 4.01!