Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 3882: 4U 1907+09; 4U 1755-33; 1983 RD

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 3881  SEARCH Read IAUC 3883
IAUC number


                                                  Circular No. 3882
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 617-864-5758


4U 1907+09
     Y. Tanaka and the Tenma Team telex: "4U 1907+09 was observed
with the x-ray satellite Tenma during Aug. 29-Sept. 7, covering
one complete binary 8.4-day period (Marshall and Ricketts 1980,
MNRAS 193, 7P).  A clear x-ray pulsation, of period ~ 438 s, was
detected throughout the observation.  A preliminary timing analysis
shows that the Doppler delay is consistent with an orbit of
8.4-day period, e = 0.2 and a sin i = 105.  Periastron passage
occurred on 1983 Sept. 1.8 UT, and the heliocentric pulse period
is 437.463 +/- 0.003 s.  The preliminary mass function, 18 +/- 4 MO,
confirms the massive nature of the primary (Schwartz et al. 1980,
A.J. 85, 549).  Further optical observations are encouraged."


4U 1755-33
     N. E. White and A. N. Parmar, European Space Agency; and
K. O. Mason, Mullard Space Science Laboratory, report that a
9.7-hr GSPC ESOSAT observation on Aug. 7 revealed three ~ 30-min
dips equally separated by 4.4 +/- 0.2 hr.  With considerable
variability and no obvious energy dependence, the flux was reduced by ~
20 percent during each event.  The events are reminiscent of the
50-min absorption dips seen from 4U 1916-05 (cf., e.g., White and
Swank 1982, Ap.J. 253, L61).  4U 1755-33 is one of several x-ray
sources that have unusually soft spectra when compared to the vast
majority of galactic sources (IAUC 3806).  Observations of the
mag-19 optical counterpart are urged.


1983 RD
     Ephemeris continuation from MPC 8214:

     1983/84 ET  R.A. (1950.0) Decl.      p        r      Mag.

     Nov.  2     4 55.41    -18 31.5    0.223    1.149    16.0
          12     4 53.88    -17 41.5
          22     4 48.55    -15 46.9    0.310    1.244    16.6
     Dec.  2     4 42.31    -13 01.9
          12     4 37.37    - 9 43.4    0.428    1.361    17.4
          22     4 35.13    - 6 10.6
     Jan.  1     4 36.02    - 2 40.1    0.595    1.490    18.3
          11     4 40.06    + 0 38.1
          21     4 46.95    + 3 38.0    0.815    1.622    19.3


1983 October 25                (3882)              Brian G. Marsden

Read IAUC 3881  SEARCH Read IAUC 3883


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


Valid HTML 4.01!