Circular No. 3373 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 COMET BRADFIELD (1979c) D. Herald, Kambah, near Canberra, reports the following precise positions: 1979 UT R. A. (1950) Decl. m1 June 25.33368 8 37 43.55 - 0 14 54.2 10-11 25.39410 8 37 44.40 - 0 10 42.5 U SCORPII Y. Kozai, Tokyo Astronomical Observatory; and J. Mattei, American Association of Variable Star Observers, communicate the following observations of the outburst of this recurrent nova (but see also IAUC 3341 and 3343): 1979 UT Mag. Observer June 23.550 8.7* Hiroaki Narumi 23.628 8.8 Yoshiyuki Kuwano (Tri-X film) 24.906 9.4 Tom Cragg (Anglo-Australian Obs.) *incorrectly given as 6.7 on the telegram C. Whitney, Center for Astrophysics, provides the following photoelectric observations obtained with the 40-cm reflector at Harvard's Agassiz Station: June 26.16 UT, V = 10.30, U-V = -0.71, B-V = -0.13, V-R = +1.15, V-I = +1.93. NOVA IN NGC 5272 B. Mayer, PROBLICOM Sky Survey, reports that Steve Wasserbaech and Jerry Johnson, Salt Lake City, have discovered a novalike star in the globular cluster NGC 5272 = M3. The star, located 22" due south of the cluster center, was observed at V ~ 12 (+/- 0.5) on May 31. It was ~ 2 magnitudes fainter in April, according to photographs taken both by Mayer and Wasserbaech. On June 25 its V magnitude was 15 +/- 0.5, according to W. Liller, who also observed the star with a Reticon spectrograph at the Mount Hopkins Observatory. Its spectrum from 4500 to 7000 A appears typical of a nova near maximum with only Balmer lines visible in absorption. 1979 June 27 (3373) Daniel W. E. Green
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