Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 3514: 1980n; H 2252-035; 1980k

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 3513  SEARCH Read IAUC 3515
IAUC number


                                                  Circular No. 3514
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


PERIODIC COMET REINMUTH 2 (1980n)
     M. P. Candy, Perth Observatory, reports that P. Jekabsons has
recovered this comet as follows:

     1980 UT             R. A. (1950) Decl.        m1
     Sept.10.49722    17 12 11.54   -24 25 52.0    18
          11.50524    17 13 25.84   -24 24 04.6

The object is diffuse, with condensation but without tail, and in
close agreement with the prediction on MPC 5043.


H 2252-035
     N. E. White and F. E. Marshall, Goddard Space Flight Center,
write: "A HEAO-A2 observation made on 1978 Dec. 5 reveals that the
x-ray flux of H 2252-035 is modulated with a period of 805 +/- 5 s.
The modulation is sinusoidal with a peak-to-mean amplitude of ~ 40
percent.  The optical period of 859 s (cf. IAUC 3511) is a beat
between the x-ray pulse period and the 3.59-hr orbital period."

     J. Patterson and M. Garcia, Harvard-Smithsonian HEAO A-3 Team,
communicate: "Analysis of HEAO A-3 data from a pointed observation
on 1978 Dec. 5 and of Einstein IPC data on 1979 May 25 confirms the
existence of x-ray pulsations.  The pulsed fraction is 85-100
percent, and the wave form is closely sinusoidal.  The period is not
well determined, but the best fit is obtained for P = 804.7 +/- 4 s,
consistent with the period reported by White and Marshall (above).
This is almost certainly the rotation period of the compact star.
Comparison with the optical data indicates that the 859-s optical
pulsations probably arise from reprocessing of x-rays in the
atmosphere of the secondary.  The x-ray spectrum indicates a
bremsstrahiung temperature ~ 8 keV, as is typical for cataclysmic
variables."


COMET CERNIS-PETRAUSKAS (1980k)
     Total visual magnitude estimates and coma diameters: Aug.
31.19  UT, m1 = 12.6, d = 1'.5 (D. Machholz, San Jose, CA, 0.25-m
reflector); Sept. 7.20, 12.9, 1'.5 (Machholz); 8.04, 11.5, 2'.2 (3.
Bortle, Stormville, NY, 0.32-m reflector); 9.04, 11.4, 2'.2 (Bortle);
12.04, 11.6, ~ 2' (Bortle).


1980 September 16              (3514)              Brian G. Marsden

Read IAUC 3513  SEARCH Read IAUC 3515


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


Valid HTML 4.01!