Fujii-san has reported the following sepctrum of V598 Pup. The FWHM of Halpha was 2300 km/s. [O III] 5007, 4959 lines were observed in strong emission. The overall feature suggests that the object is a fast nova currently in typical nebular phase. http://www1.harenet.ne.jp/~aikow/etc/v598_pup_20071120.gif