Circular No. 4885 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 or GREEN@CFA.BITNET MARSDEN or GREEN@CFAPS2.SPAN V745 SCORPII J. Spyromilio and P. Whitelock, Anglo-Australian Observatory; P. Meikle and G. Varani, Imperial College, London; and M. Feast, South African Astronomical Observatory, telex: "Spectra (resolution 500) of V745 Sco were obtained at the Anglo-Australian Telescope in the J, K, and L' windows on Oct. 11. The spectra show strong He (1083 nm) and weaker Paschen beta and Brackett gamma, all in emission. The continuum in the J window rises toward longer wavelengths. The first overtone of CO is strong in absorption and presumably results from the companion star, possibly an M star (cf. IAUC 4844). The L' spectrum is approximately flat and featureless but of poorer signal-to-noise ratio. Photometry at SAAO yields: Aug. 28, J = 9.98, H = 8.74, K = 8.20, L = 7.51; Oct. 17, 9.99, 8.71, 8.23, 7.79." UV PERSEI A. Udalski, York University, Toronto, and Warsaw University Observatory; and J. A. Mattei, AAVSO, report: "The dwarf nova UV Per is undergoing a long outburst. The star has been brighter than mag 13 since Oct. 16 (cf. IAUC 4880). Three sets of observations were obtained using the 0.61-m/0.48-m twin photometric system of the David Dunlap Observatory during Oct. 22-24. Periodic light variations (superhumps) with an amplitude up to 0.3 mag were discovered. Based on 10 maxima timings, the preliminary superhump period is about 95.5 min. The discovery of superhumps during the long eruption (superoutburst) indicates that UV Per is a new member of the SU UMa subclass of dwarf novae." Further visual magnitude estimates: Oct. 18.75 UT, 11.7 (P. Schmeer, Bischmisheim, W. Germany); 19.74, 12.5 (E. Schweitzer, Strasbourg, France); 21.98, 12.7 (G. Dyck, N. Dartmouth, MA); 22.20, 12.1 (J. Griese, Rocky Hill, CT); 22.75, 13.0 (Schweitzer); 23.13, 12.8 (M. Heifner, Denver, CO); 23.29, 11.9 (Griese); 24.40, 11.9 (C. Scovil, Stamford, CT); 26.00, 12.9 (A. Mizser, Budapest, Hungary). R CORONAE BOREALIS Visual magnitude estimates by J. E. Bortle, Stormville, NY (cf. IAUC 4860): Sept. 25.15 UT, 7.6; Oct. 5.1, 6.9; 24.1, 6.6. 1989 October 26 (4885) Daniel W. E. Green
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