SIMBAD references

M. Fujii, Okayama, Japan, reports that a low-resolution spectrogram (range 400-830 nm) of V407 Cyg was taken on Mar. 13.793 with a 40-cm telescope. The spectrum shows strong Balmer series, Fe II (multiplets 27, 37, 42, 48, 49, 55, 74), He I (587.6, 667.8, 706.5 nm), and O I (777.4 nm) emission lines. The FWHM of the H_alpha emission line is 1600 km/s. The spectrum can be seen at http://otobs.org/FBO/fko/nova/v407_cyg_20100313.gif.