SIMBAD references

Following posting on the Central Bureau's unconfirmed-objects webpage, H. Naito and S. Narusawa, Nishi-Harima Astronomical Observatory, report that a low-resolution spectrogram (range 410-670 nm; resolution 1500 at H_alpha) of this possible nova, obtained on Mar. 20.84 UT with the 2.0-m NAYUTA telescope (+ MALLS), shows Balmer-lines having P-Cyg features and Fe II lines (multiplets 42, 49, 74), suggesting that the variable is a "Fe II"- type nova. The FWHMs of the H_alpha, H_beta, and H_gamma emissions are 920, 810, and 790 km/s, and the displacement of the P-Cyg absorptions from the Balmer emission peaks is 940, 820, and 830 km/s, respectively.