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 probable nova reported on CBET 2183 was obtained with the BAO 1-m telescope on Feb. 23.88 UT. This shows prominent H-alpha emission with P-Cyg absorption upon a red continuum. The FWHM and equivalent width of the H-alpha emission component are about 1800 km/s and 70 nm, respectively, and 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 show that the new object is a "Fe II"-type nova.