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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