V2275 Cyg spectrum by Fujii M. Fujii (Fujii Bisei Observatory) has further provided a spectrum of V2275 Cyg (Nova Cyg 2001-2) taken on Aug. 22.50 UT. The Balmer lines have become more intensive compared to the spectrum taken on the first night (Ayani, Bisei Observatory). The FWHM of the H-alpha line is 3100 km/s. The spectrum can be seen at: http://vsnet1.harenet.ne.jp/~aikow/v2275_cyg.gif Based on the clear presence of Fe II multiplets, Fujii concluded that the nova is a typical "Fe II-type" nova. Relayed from M. Fujii