SIMBAD references

K. Kinugasa, H. Takahashi, and O. Hashimoto, Gunma Astronomical Observatory (GAO), write that a low-dispersion spectrum (range 420-850 nm, resolution about 500) of this object, taken on Apr. 29.745 UT with the GAO 1.5-m telescope (+ GLOWS), shows broad (FWHM about 4000 km/s) Balmer and O I (777.4-, 822.7-, and 844.6-nm) emission lines. Both H_alpha and H_beta have asymmetric line profiles with a blue peak. Several emission lines of He I and N II are also seen. The features indicate that the object is a He/N nova in a declining phase. Their spectrum can be viewed at the following website URL: http://tinyurl.com/37r6yhj.