Possible Nova in Pup: spectrum by Fujii M. Fujii (Fujii Bisei Observatory) reports the spectrum of the possible nova on Puppis. The spectrum was taken on Dec. 31.7, using a 28-cm refelctor. The spectrum is rich in emission lines. Fujii identified prominent emission lines of Fe II (multiplets 19F, 34F, 42, 74) and He I 587.6 nm, while H-beta emission is weak or absent. Fujii suggests that the object is a somewhat peculiar nova. The reduced spectrum is posted at: http://vsnet1.harenet.ne.jp/~aikow/p_n_p.gif. Fujii's report was sent to the CBAT.