Read IAUC 3374
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
Read IAUC 3374
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