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Circular No. 7176 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Mailstop 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions) BMARSDEN@CFA.HARVARD.EDU or DGREEN@CFA.HARVARD.EDU (science) URL http://cfa-www.harvard.edu/iau/cbat.html ISSN 0081-0304 Phone 617-495-7244/7440/7444 (for emergency use only) NOVA VELORUM 1999 Independent visual discoveries of a bright nova have been made by Peter Williams, Heathcote, New South Wales (via S. Lee and A. Pearce), at m_v = 3.1 on May 22.396 UT and by Alan C. Gilmore, Mount John University Observatory, on May 22.451. Lee provides the following position from Anglo-Australian Telescope (AAT) encoders: R.A. = 10h44m49s.5, Decl. = -52o25'35" (equinox 2000.0). Lee reports that a low-dispersion spectrogram taken by Lewis, Colless, Cannon, Bridges, and himself with the AAT (+ fiber spectrograph on 2dF; 1-s exposure, mirror stopped down to 2.5 m) shows H-alpha and H-beta in narrow emission with a strong P-Cyg profile. An echelle spectrogram (10-min exposure centered on May 22.500) of the apparent nova by K. R. Pollard and J. A. McSaveney with the Mt. John 1-m telescope shows H-alpha with blueshifted absorption and slightly redshifted emission. Gilmore provides the following photometry obtained with the Mount John 0.6-m reflector (comparison star HR 4167 = p Vel, with assumed V = 3.84, U-B = +0.07, B-V = +0.30, V-R = +0.20, V-I = +0.30): May 22.488, V = 2.88, U-B = -0.27, B-V = +0.24, V-R = +0.16, V-I = +0.28; 22.574, 2.85, -0.27, +0.28, +0.19, +0.27; 22.599, 2.84, -0.25, +0.29, +0.23, +0.33; 22.635, 2.80, -0.26, +0.31, +0.23, +0.33. P. M. Kilmartin reports that a 1-s CCD (over)exposure on May 22.50 with the 0.6-m Boller & Chivens Cassegrain reflector at Mount John yields the following position end figures: 48s.1, 32" (four stars, mean residual 2".68 in R.A., 0".43 in Decl.). Pearce provides the following visual magnitude estimates: May 22.42-22.52, 3.0; 22.54-22.58, 2.9. Pearce notes that there appears to be nothing obvious on the Digital Sky Survey image at the nova's position. P. Caldwell, Geelong, Victoria, reports m_v about 2.8 (close to or slightly fainter than the brightness of mu Vel) during May 22.50-22.53. COMET C/1999 K4 (LINEAR) An apparently asteroidal object found by LINEAR (discovery observation below; further observations and orbit on MPEC 1999-K24), and posted on The NEO Confirmation Page, has been reported as cometary by M. Hicks (Table Mountain; faint coma of diameter about 5" on May 21) and by C. W. Hergenrother and A. E. Gleason (Catalina 1.5-m reflector; highly condensed coma with a faint 10"-15" tail in p.a. 170 deg on May 22). 1999 UT R.A. (2000) Decl. m2 May 17.32636 16 05 48.69 + 5 45 19.7 18.7 (C) Copyright 1999 CBAT 1999 May 22 (7176) Daniel W. E. Green
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