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    [Fwd: CBET 2050: 20091126 : POSSIBLE NOVA IN ERIDANUS]

    From: Joe Patterson <jop_at_astro.columbia.edu>
    Date: Wed, 25 Nov 2009 21:12:14 -0500
    Dear CBAers,
    
    With a galactic latitude of 31 degrees and a possible range of 8 mag, 
    this could be an awfully interesting object.  It could be a very nearby 
    dwarf nova, or a really distant nova.  Or maybe something else... but 
    it's very much worth a looksee to figure out if the new object really is 
    that 15th mag star.  If it is, then I highly recommend a photometric 
    run!  And if not, well, it's still worth some study.
    
    joe
    
    -------- Original Message --------
    Subject: CBET 2050: 20091126 : POSSIBLE NOVA IN ERIDANUS
    Date: Wed, 25 Nov 2009 20:52:31 -0500
    From: IAUC mailing list <quai@cfa.harvard.edu>
    To: iauc@libraries.cul.columbia.edu
    
                                                       Electronic Telegram 
    No. 2050
    Central Bureau for Astronomical Telegrams
    INTERNATIONAL ASTRONOMICAL UNION
    M.S. 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
    IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions)
    CBAT@CFA.HARVARD.EDU (science)
    URL http://www.cfa.harvard.edu/iau/cbat.html
    
    
    POSSIBLE NOVA IN ERIDANUS
          Hitoshi Yamaoka, Kyushu University, reports the discovery by K. 
    Itagaki
    (Yamagata, Japan) of a possible nova (mag 8.1) caught on Nov. 25.536 UT with
    his 0.21-m patrol system.  A confirming image taken by Itagaki on Nov. 
    25.545
    with a 0.60-m reflector shows the object at R.A. = 4h47m54s.21, Decl. =
    -10d10'43".1 (equinox 2000.0).  Itagaki notes that there is a faint (mag 
    about
    15) object near this position on his archival patrol images.  Yamaoka 
    suggests
    that it might be the brightening of a 15th-mag blue star that is 
    contained in
    many catalogues (USNO-B1.0 position end figures 54s.19, 42".9), noting that
    the amplitude of seven magnitudes is rather large for a dwarf nova, but
    somewhat small for a rapid classical nova.  Yamaoka adds that the ASAS-3
    system (Pojmanski 2002, Acta. Astron. 52, 397) also detected this object at
    the following V magnitudes:  Nov. 10.236 UT, [14.0:; 19.241, 7.34; 22.179,
    7.98; 24.269, 8.12.
    
    
    NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
           superseded by text appearing later in the printed IAU Circulars.
    
                              (C) Copyright 2009 CBAT
    2009 November 26                 (CBET 2050)              Daniel W. E. Green
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    Received on 25 Nov 2009