SIMBAD references

A. Arai, T. Kajikawa, and M. Nagashima, Kyoto Sangyo University, write that they performed low-dispersion optical spectroscopic observations (range 400-750 nm; R about 600) of PNV J16551100-3838120 on June 2.68 UT using the 1.3-m Araki telescope (+ LOSA/F2) under a hazy sky. The spectrum shows a broad H-alpha (FWZI about 4600 km/s) with an asymmetric profile and O I (777.4 nm) on a highly-reddened continuum. No visible He or Fe II lines exist in the spectrum. These features suggest that the object is a classical nova in outburst with high interstellar reddening. The spectrum is posted at website URL http://www.cc.kyoto-su.ac.jp/~kao/blog/index.php/view/98.