SIMBAD references

Maehara also communicates the following report by M. Fujii (Okayama) and concludes that the object seems likely to be an He/N-class nova: "A spectrum (range 380-880 nm) of the object obtained on Nov. 26.49 UT shows Balmer (FWHM of H_alpha emission 3200 km/s), He I (447.1, 501.6, 587.6, 667.8, 706.5 nm), N III (464.0 nm), Na I D (589.2 nm), O I (777.3, 844.6 nm) and Mg II (823.2 nm) emission lines. See also http://otobs.org/FBO/fko/nova/pn_eri_20091126.gif ."