[vsnet-alert 233] Re: Possible Nova

[Ohshima Osamu <ohshima@bao.go.jp>]

   I took spectrograms of possible nova Oph ;
      RA 17 57 48.6  DEC 4 41 03 (2000)
  with CCD spectrograph + the BAO 1.0-m telescope Sept 12.41UT. 
  The object has not Balmer P Cyg profiles but red continuum with TiO bands.
  The object may move from south, GSC425:184 = The Barnard Star ! 
  as Mr. Nakamura of Kuma-Kogen Observatory poits out.

  Thank you

  Osamu Ohshima
  Bisei Astronomical Observatory

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