[vsnet-alert 14747] Spectroscopy of the Nova Sgr 2012 No.4

[K. Imamura]

Spectroscopy of the Nova Sgr 2012 No.4

   We have obtained a spectrum (R~400) of the Nova Sgr 2012 No.4 
(CBET3166) on July 8.578 (UT), using the DSS-7 spectrometer 
attached to the 0.28-m Schmidt-Cassegrain telescope at the OUS 
Observatory. Emission lines of Balmer series, Fe II multiplets 
(27, 37, 38, 42, 46, 48, 49, 55 and 74), Na I D and O I (7773) 
can be seen in the spectrum. The FWHM of H-alpha is 
approximately 1800 km/s.

Our spectra can be seen in the following:
  http://tnblab.blog7.fc2.com/blog-entry-319.html

--
Kazuyoshi Imamura (Okayama Univ. of Sci. team)