Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 5880: SGR 1806-20; V1974 Cyg; NOTICE TO SUBSCRIBERS; N Aql 1993

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 5879  SEARCH Read IAUC 5881

View IAUC 5880 in .dvi or .ps format.
IAUC number


                                                  Circular No. 5880
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)


SGR 1806-20
     Y. Tanaka, Institute of Space and Astronautical Science, on
behalf of the ASCA Team, communicates: "Following the notice of new
activity of SGR 1806-20 (IAUC 5875), we observed the source with
ASCA between Oct. 9.67 and 11.58 UT.  Quick-look data show an
anomalous increase of counts (burst) in a 4-s time bin, which includes
the time of occurrence of a gamma-ray burst (at Oct. 9.934) detected
by the BATSE instrument on the Compton Gamma Ray Observatory
from SGR 1806-20 (private communication by C. Kouveliotou).  We
discovered in the same observation a new x-ray source at R.A. =
18h05m42s, Decl. = -20o25'10" (equinox 1950.0), with an error-circle
radius of 1', coincident with a radio source reported on IAUC
5879.  The source intensity is about 0.2 mCrab (0.5-10 keV) with a
heavy absorption.  Preliminary analysis localized the position of
the ASCA burst into a cell of 3' x 6', which includes the new x-ray
source.  We tentatively identify this radio/x-ray source to be the
counterpart of SGR 1806-20."


V1974 CYGNI
     J. A. DeYoung and R. E. Schmidt, U.S. Naval Observatory,
report: "Time-resolved Kron-Cousins I-band photometry of V1974 Cyg
(N Cyg 1992) on Oct. 6.99-7.08, 7.98-8.15, 10.98-11.15, and 12.98-
13.18 UT shows a modulation with a period of 1.95 hr and a peak-to-
peak amplitude of 0.16 +/- 0.02 magnitude.  A linear least-squares
fit using the seven times of observed minima gives a period of
0.08123 +/- 0.00003 day."


NOTICE TO SUBSCRIBERS
     Subscribers to the Computer Service who have e-mail access are
advised that, in addition to the login information they already
have, use of the Username IAUMAIL (with the password information
they already have) will allow them to MAIL to themselves specific
Circulars that may have failed to arrive in the original e-mail
transmission.


NOVA AQUILAE 1993
     Further CCD photometry by H. Mikuz, Ljubljana, Slovenia (cf.
IAUC 5818, 5838):  Aug. 21.91 UT, V = 13.93 +/- 0.05; Oct. 4.81,
13.29 +/- 0.05.


1993 October 15                (5880)            Daniel W. E. Green

Read IAUC 5879  SEARCH Read IAUC 5881

View IAUC 5880 in .dvi or .ps format.


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


Valid HTML 4.01!