SIMBAD references

H. Maehara, Kwasan Observatory, Kyoto University, reports that A. Arai and M. Isogai (Kyoto Sangyo University) observed the nova with a 28-cm reflector and a low-resolution spectrograph on Nov. 26.5 UT. The nova shows a broad H_alpha emission line with a FWHM around 3200 km/s and a notable blue continuum. H_alpha and H_beta emission lines clearly show asymmetric profiles. N III (464.0 nm), N II (567.9 nm), and He I (587.6 nm) emission lines were strong. A blended line of N II (500.1 nm) and He I (501.6 nm) was also seen. These spectral features indicates that the object is a He/N nova.