SIMBAD references

K. Ayani, Bisei Astronomical Observatory (BAO), writes that low-resolution spectra (range 380-800 nm; resolution 0.55 nm at H_alpha), obtained with the BAO 1.01-m telescope on Mar. 16.8 UT, show that this variable is a nova. The spectra show Balmer and Fe II absorption lines on a red continuum. The H_alpha line has a P- Cyg profile whose absorption bottom is blueshifted by 1200 km/s with respect to the emission peak.