Nova Sgr 2002: spectroscopy by Fujii M. Fujii (Fujii Bisei Observatory) obtained the spectrum of the supposed nova (Nova Sgr 2002) on Apr. 18.80 UT. http://vsnet1.harenet.ne.jp/~aikow/p_nova_sgr_0418.gif Fujii reports that the following emission lines are present: strong H-alpha (FWHM=2800km/s), H-beta, Fe II (37,38,42,49,55,74), Na I (5890) and He I(7065). The object is an Fe II-class nova.