Circular No. 3292 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 1630-47 S. Holt, L. Kaluzienski, R. Mushotzky, F. Boldt and P. Serlemitsos, Goddard Space Flight Center, report that recent observations of the galactic plane in Norma with the Ariel 5 all-sky monitor reveal the presence of a bright source at a position consistent with that of the recurrert transient x-ray source 4U 1630-47. The 3-6-keV flux measured on Oct. 8 (shortly after the source entered the field of view of the detector) was approximately one-third that of the Crab Nebula (assuming an intensity for the nearby bright variable source 4U 1642-45 equal to the observed Uhuru maximum). Quick-look data obtained with the HEAO-A2 experiment on Sept. 6 also show a source at approximately this intensity roughly consistent with the position of 4U 1630-47. The latest outburst from this source was observed in 1977 Nov. (IAUC 3144), with subsequent detections reported in 1978 Mar. (IAUC 3197) and June (IAUC 3227). This, if the identification of the above source with 4U 1630-47 is correct, the present observations are indicative of a prolonged emission plateau or extended secondary maximum in the decay of this object. In either case, this would represent the longest-lived flaring episode of a 'transient' source yet observed. CYGNUS X-2 D. Crampton and A. Cowley, Dominion Astrophysical Observatory, write: "New spectroscopic observations of Cyg X-2 show the orbital period to be 9.8 days. A phase-dependent spectral-type variation (A5-F2) implies strong x-ray heating on the optical star. It is expected that a corresponding photometric variation of up to a few tenths of a magnitude should be present. Superior conjunction occurs at: JD 2443161 + 9.8431 E." IMPORTANT NOTICE It seems that the preaddressed cards for some recent Circulars have been mixed up, with the result that subscribers have received two copies of some issues and none of others. The problem was particularly acute with IAUC 3281-3283 and 3285-3286, and we are still trying to assess the situation. It would be helpful if subscribers writing for missing issues would enclose any duplicate issues they might have received. 1978 October 18 (3292) Brian G. Marsden
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