SIMBAD references

Maehara adds that A. Arai, T. Komatsu, M. Yamanaka, M. Sasada, and R. Itoh (Higashi-Hiroshima Observatory, Hiroshima University) obtained a spectrogram of the nova with the High Speed Spectrograph attached to the 1.5-m KANATA telescope on Aug. 7.63 UT; the Balmer lines (H-alpha and H-beta) and Fe II emission lines are seen in their spectrum. H-alpha emission line shows an asymmetric profile; the FWHM of the H-alpha emission line is about 2100 km/s. Their spectrum can be found at http://kanatatmp.g.hatena.ne.jp/kanataobslog/20090807. Maehara notes that these observations confirm that the object is a nova.