SIMBAD references

A. Arai, T. Kajikawa, C. Naka, Kyoto Sangyo University, write that they performed low-resolution optical spectroscopic observations (R about 580) of PNV J16364440-4132340 on Sept. 7.42 UT using the Araki telescope at Koyama Astronomical Observatory. The spectrum exhibits broad Balmer emissions and Fe II multiplet emissions on a highly reddened continuum light. The H-alpha emission line shows an asymmetric profile with FWZI about 6000 km/s. Other significant features are invisible in the spectrum (posted at website URL http://www.cc.kyoto-su.ac.jp/~kao/blog/index.php/view/127). These features suggest that the object is an "Fe II"-type classical nova, highly reddened by the interstellar medium.