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Circular No. 5650 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Telephone 617-495-7244/7440/7444 (for emergency use only) TWX 710-320-6842 ASTROGRAM CAM EASYLINK 62794505 MARSDEN@CFA or GREEN@CFA (.SPAN, .BITNET or .HARVARD.EDU) GRO J0422+32 T. Mazeh, E. M. Leibowitz, S. Hemar, and H. Mendelson, Wise Observatory, Tel Aviv University; and R. E. McCrosky, Oak Ridge Observatory, Harvard-Smithsonian Center for Astrophysics, report: "The optical counterpart of GRO J0422+32 has been monitored at Wise and Oak Ridge Observatories on more than 20 nights since Aug. 28, including CCD B photometry for a few hours each night, with a time resolution of 4-5 min, showing that the star's average brightness declined at a rate of about 0.01 mag/day. So far, more than a thousand exposures have been analyzed. On every night, the star displayed erratic eruptions on timescales of 1-2 hr, with a typical amplitude of 0.1 mag. This variation is reflected in the power spectrum of the whole data set through a QPO-like feature at frequencies close to 0.5 hrE-1. The power spectrum also reveals a power-law rise toward the low-frequency end of the spectrum. We find no evidence for 4.5- or 5-hr stable periodicity in our data." PERIODIC COMET SWIFT-TUTTLE (1992t) G. P. Tozzi and G. Calamai, Osservatorio Astronomico Arcetri, Florence, report the following magnitudes obtained with the Italian National Infrared Telescope TIRGO (28" diaphragm), showing a sharp increase in infrared brightness over 24 hr: Nov. 6.7 UT, J = 8.85 +/- 0.05, H = 8.45 +/- 0.05, K = 8.23 +/- 0.05; Nov. 7.7, 8.25 +/- 0.10, 7.90 +/- 0.10, 7.80 +/- 0.10. PERIODIC COMET BREWINGTON (1992p) Ephemeris extension from orbital elements on MPC 21081: 1992/93 R. A. (2000) Decl. Delta r Elong. Phase m1 Nov. 14 9 36.10 +32 36.1 1.990 2.315 96.1 25.1 15.1 24 9 42.02 +32 31.7 1.937 2.384 104.5 23.6 15.5 Dec. 4 9 44.47 +32 39.7 1.886 2.454 113.6 21.6 16.0 14 9 43.30 +32 58.1 1.844 2.524 123.4 19.0 16.4 24 9 38.48 +33 23.0 1.815 2.594 133.8 15.9 16.9 Jan. 3 9 30.32 +33 48.3 1.803 2.665 144.4 12.4 17.3 13 9 19.54 +34 06.5 1.814 2.735 154.5 8.9 17.8 23 9 07.27 +34 11.1 1.853 2.806 162.1 6.2 18.3 Feb. 2 8 54.91 +33 58.3 1.920 2.876 162.8 5.8 18.8 12 8 43.80 +33 27.8 2.016 2.946 156.1 7.8 19.3 22 8 34.87 +32 42.7 2.140 3.016 146.7 10.4 19.8 Mar. 4 8 28.67 +31 47.0 2.288 3.085 136.7 12.7 20.4 14 8 25.30 +30 44.9 2.455 3.154 126.9 14.6 20.9 24 8 24.57 +29 39.5 2.640 3.223 117.4 15.9 21.4 Total visual magnitudes from H. Mikuz, Ljubljana, Slovenia (0.2-m reflector): Sept. 8.13 UT, 11.2; 26.14, 12.3 (CCD); Oct. 9.14, 14.4. 1992 November 10 (5650) Daniel W. E. Green
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