SIMBAD references

Yamaoka also forwards a report from M. Fujii (Kurashiki, Okayama, Japan), who obtained a low-resolution spectrum of this object on Feb. 19.86 UT with his 0.28-m telescope. In addition to the Balmer lines with P-Cyg profile, Fujii noticed a Fe II (37, 42, 49) emission feature, which suggests that the variable is a "Fe II class" nova. He measured that the blueshift of the H-alpha absorption minimum from the emission peak is about 700 km/s, and the equivalent width of Na I D lines is about 0.4 nm. Fujii's spectrum can be seen at the following website URL: http://otobs.org/FBO/fko/nova/pn_oph_20100219.gif.