SIMBAD references

K. Ayani, Bisei Astronomical Observatory (BAO), reports that low-dispersion spectra (range 463-690 nm; resolution 0.54 nm at H_alpha) of the apparent nova, obtained on Nov. 21.75 at the BAO 1.01-m telescope, shows H_alpha and H_beta lines with P-Cyg profiles. Preliminary analysis of the H_alpha emission (without decomposition of the absorption component) yields FWHM = 650 km/s and equivalent width 0.6 nm, the minimum of the H_alpha P-Cyg absorption being blueshifted by 860 km/s with respect to the emission peak. Absorption of Fe II (multiplet 42) lines are clearly seen.