SIMBAD references

K. Ayani, Bisei Astronomical Observatory (BAO), writes that a low-resolution spectrum (range 400-800 nm; resolution 0.5 nm at H_alpha) of the new variable, obtained with the BAO 1-m telescope on Feb. 23.88 UT, shows prominent H_alpha emission (FWHM about 1800 km/s; equivalent width 70 nm) with P-Cyg absorption upon a red continuum; the absorption bottom is blueshifted by 1600 km/s with respect to the emission peak. The spectrum also shows emission lines of H_beta and Fe II (multiplet 42), which are weak and probably due to large interstellar extinction. These features suggest that the new object is a "Fe II"-type nova.