Circular No. 3450 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 GK PERSEI J. E. Nelson, Lawrence Livermore Laboratory, communicates: "The imaging proportional counter on the Einstein Observatory will be used to monitor the x-ray cataclysmic variable GK Per on 1980 Feb. 14, 15 and 16 UT for three hours each night. Interested optical and infrared observers should telephone F. A. Cordova (505-667-3904) or myself (415-486-5913) for details." 1980 AA A. W. Harris, Jet Propulsion Laboratory, informs us that his photometric observations with the 1.5-m reflector at Mt. Wilson show that the rotation period of this object is 2.70 +/- 0.01 hours, the second shortest value found for any minor planet. On Jan. 25.3 UT he obtained V (mean) = 14.08, B-V = +0.81 +/- 0.02, U-B = +0.37 +/- 0.05. The full amplitude in V was 0.10 mag. Observations were also made on Jan. 24. The resulting B(1,0) = 20.1. COMET BRADFIELD (1979l) R. M. West and G. F. O. Schnur, European Southern Observatory, report that a series of short exposures with the 3.6-m reflector show a faint nuclear condensation, ~ 1" (150 km) in diameter. On Jan. 23.3 UT a faint, straight tail was also seen, together with some features (streamers?) near the nucleus. By Jan. 24.1 UT the tail had become rquch broader and showed internal structure. The following UBV photometric observations were made by H. J. Schober with the Bochum 0.61-m telescope at the European Southern Observatory, using a diaphragm of 45" centered on the nucleus; integration times were 10-30 s. Jan. 23.354 UT, V = 9.39 +/- 0.02, B-V = +0.39 +/- 0.02, U-B = -0.18 +/- 0.03; 24.111, 9.49 +/- 0.04, +0.37 +/- 0.04, -0.26 +/- 0.04; 25.083, 9.50 +/- 0.03, +0.36 +/- 0.03, -0.14 +/- 0.05. Selected visual observations: Jan. 25.83 UT, m1 = 4.7, coma diameter D = 15' (J. C. Bennett, Pretoria, 0.12-m refractor); 27.04, 4.0, 25' (P. Maley, Houston, 7 x 50 binoculars); 28.02, 4.7, 12' (C. S. Morris, Harvard, MA, 20 x 80 binoculars); 28.96, 6.0, 20' (S. O'Meara and P. Collins, Cambridge, MA, 11 x 80 binoculars; some tail/streamer activity, 0.23-m refractor); 29.75, 5.5, 15' (5. Baroni, M. Cavagna and G. Clerici, Milan, 15 x 80 binoculars). 1980 January 30 (3450) Brian G. Marsden
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