Circular No. 3687 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 3A 0729+103 I. M. McHardy and J. P. Pye, University of Leicester; A. P. Fairall, B. Warner, S. Allen and M. Cropper, University of Cape Town; and M. J. Ward, Institute of Astronomy, Cambridge, report the identification of the x-ray source 3A 0729+103 with a newly discovered catac1ysmic variable of mag ~14.5, based on an arcmin-precision position obtained from an Einstein IPC guest observation. Extensive photometry in white light with 10-s time resolution shows stochastic flickering and occasional flares (of amplitude 5 percent) superimposed on a coherent sinusoidal pulsation of period 913s.48 and mean amplitude 12 percent. There may be an orbital modulation of period 3.75 hr and amplitude 8 percent. The x-ray observations also show evidence of a period of ~ 900-1000s. Low resolution optical spectra show broad He and Balmer lines, up to H11, in emission. The lines have fwzi of ~ 1600 km/s and vary in strength through the 913-s period, with most variation being noticed in the higher Balmer lines. High-resolution optical spectra show that many emission lines have multiple components. The star is at R.A. = 7h28m44s.4, Decl. = +10o02'46" (+/- 1".5, equinox 1950.0). SY MUSCAE P. Whitelock, South African Astronomical Observatory, telexes: ~The symbiotic star SY Mus does not appear to have undergone any gross changes in the infrared that might correspond with those reported in the ultraviolet (IAUC 3657). On Feb. 4 the JHKL magnitudes were as follows: J = 5.93, H = 4.95, K = 4.62, L = 4.37 (with standard errors of +/- 0.05). These values are not significantly different from those measured in 1976." PERIODIC COMET SCHWASSMANN-WACHMANN 1 J. Bortle, Stormville, NY, and J.-C. Merlin, Le Creusot, France, have independently reported a new outburst of this comet. Available visual magnitude estimates are: Apr. 13.08 UT, 13.1 (Bortle, 0.32-m reflector); 13.9, 11.5 (Merlin); 14.19, 12.8 (C. S. Morris, Harvard, MA, 0.25-m reflector); 14.87, 11.6 (G. M. Hurst, Wellingborough, England, 0.26-m reflector); 15.13, 12.6 (Morris). Bortle adds that the coma, of diameter 0'.25, was tiny, dense, but not particularly condensed. 1982 April 16 (3687) Brian G. Marsden
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