According to M. Fujii, Nova Sct 2005 = V476 Sct is shown to be a typical Fe II-type nova. Spectrum on Oct. 6.44 UT: http://www1.harenet.ne.jp/~aikow/etc/nova_sct_20051006.gif The FWHM of Halpha is 1700 km/s. [O I] line is strong. The nova also shows a substantial reddening, as suggested from photometry.