SIMBAD references

K. Kinugasa, H. Takahashi, S. Honda, H. Taguchi, and O. Hashimoto, Gunma Astronomical Observatory (GAO), write that a low-resolution spectrum (range 420-800 nm; resolution 1.0 nm), obtained with the GAO 1.5-m telescope (+ GLOWS) on Dec. 15.4 UT, confirms that the object announced on CBET 2075 is a nova, showing H_alpha emission (FWHM about 1000 km/s) with a P-Cyg profile, its absorption minimum being blue-shifted by 1000 km/s with respect to the emission peak. H_beta, H_gamma, and Fe II (multiplet 42) lines also have P-Cyg profiles.