Nova Sct 2003: new spectrum by Fujii Fujii's new observation on September 13.46 UT: http://vsnet1.harenet.ne.jp/~aikow/nova_sct_20030913.gif The H-alpha line is strong (FWHM = 1200 km/s). The P Cyg profile of the Na D line is strong (the velocity of the absorption-line component with respect to the emission line component being 1200 km/s).

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