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THE ASTRONOMER Electronic Circular No 920       1995 Feb 04 13.54UT
Ed:Guy M Hurst, 16,Westminster Close, Kempshott Rise,  Basingstoke,
Hants, RG22 4PP,England. Telephone/FAX(0256)471074 Int:+44256471074
INTERNET: GMH at AST.STAR.RL.AC.UK  or    GMH at GXVG.AST.CAM.AC.UK
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NOVA CIRCINI 1995
W. Liller, Instituto Isaac Newton, Vina del Mar, reports his
discovery on a single PROBLICOM photograph (85-mm lens, orange
filter, Kodak TP film) taken Jan. 27.328 UT of a stellar object of
mv about 7.2 at the position R.A. = 14h44m58s, Decl. = -63o54'.0
(equinox 2000.0).  Nothing brighter than mag 12.0 appears at this
position on a film taken Jan. 12.336 UT.  The sharpness of the
image suggests that it is not a red variable.

S. Benetti, European Southern Observatory (ESO); and E.
Cappellaro, Padua Observatory, report that inspection of a fully-
reduced CCD spectrum (range 390--900 nm, resolution 1.3 nm) obtained
on Jan. 30.38 UT with the ESO New Technology Telescope (+ EMMI)
confirms that this object is a nova.  The spectrum is dominated by
intense emission lines of hydrogen, Fe II, and O I (777.4 and 844.6
nm).  The FWHM of H-alpha, H-beta, and H-gamma, corrected for the
instrumental resolution, is about 1500 km/s.

A. C. Gilmore, Mount John University Observatory, reports that
N Cir 1995 shows nova-like colours in photometry obtained at Mt.
John with the 0.6-m f/13 reflector (conditions were good but the
region low): Jan. 29.449 UT, V = 7.91 +/- 0.02,
U-B = -0.44 +/- 0.50, B-V = +0.38 +/- 0.02, V-R = +1.50 +/- 0.02,
V-I = +1.71 +/- 0.02 (airmass 2.14). Comparison was with two stars
in Cousins standard region F2 and nearby HR 5539. The true U-B is
likely to be more negative than obtained here.
IAUC 6130

Peter Nelson has e-mailed the following visual estimates:
Jan. 28.526 UT, 7.4 (R. Stubbings, Victoria, Australia);
     29.464,    8.1 (Peter Nelson, Victoria).

Guy M Hurst