Read IAUC 3903
Circular No. 3902
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
V0332+53
L. Stella and N. E. White, European Space Agency, report that
a more detailed analysis of the EXOSAT observations of V0332+53 on
Nov. 21 and 22 (IAUC 3893) has revealed a coherent 4.4-s modulation
of the x-ray flux. The pulse profile is variable but on the
average is a double-sine-wave pulse with a peak-to-peak amplitude
of 15 percent. This modulation was also present in an additional
observation on Nov. 26. The period is decreasing with P/P-dot = 200 +/-
50 yr from a value of 4.37534 +/- 0.00004 s on Nov. 21.22 UT. This
rate of decrease is similar to that seen from other x-ray pulsars.
The variance associated with the modulation is < 10 percent of
that caused by the stochastic flickering previously reported.
1983 VA
R. M. West, European Southern Observatory, reports the
following prediscovery observation:
1983 UT R.A. (1950.0) Decl.
Oct. 27.04763 22 32 05.51 -57 31 13.4
Improved orbital elements from observations Oct. 27-Nov. 11:
T = 1983 Dec. 17.229 ET
Peri. = 11.735 e = 0.68880
Node = 76.943 1950.0 a = 2.58208 AU
Incl. = 16.203 n = 0.237547
q = 0.80354 AU P = 4.15 years
1983/84 ET R.A. (1950.0) Decl. p r Mag.
Dec. 22 16 09.50 - 0 34.6 0.227 0.807 16.9
27 15 55.00 + 4 59.1
Jan. 1 15 46.36 + 8 38.2 0.304 0.837 17.1
6 15 41.65 +11 02.9
11 15 39.44 +12 41.6 0.382 0.893 17.3
16 15 38.70 +13 52.5
21 15 38.70 +14 47.4 0.450 0.968 17.5
26 15 38.89 +15 33.9
31 15 38.81 +16 17.0 0.505 1.056 17.7
Feb. 5 15 38.12 +16 59.5
10 15 36.56 +17 42.8 0.547 1.152 17.9
1983 December 21 (3902) Brian G. Marsden
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