SIMBAD references

H. Maehara, Kwasan Observatory, Kyoto University, writes that a low- resolution optical spectrum (range 400-800 nm, R about 200) of this nova was obtained on Oct. 27.42 UT with the 25-cm telescope of the Kwasan Observatory. The spectrum shows an H_alpha emission line that suggests this object is a classical nova. CCD images of the nova yield following magnitudes: Oct. 27.460, I_c = 8.66; 27.461, R_c = 9.29; 27.461, V = 9.90; 27.463, B = 11.06.