SIMBAD references

Akira Arai, Koyama Astronomical Observatory, Kyoto Sangyo University, reports that low-resolution (R about 550) spectroscopic observations of PNV J17474639-2335112 were obtained at the Koyama Astronomical Observatory on Jan. 28.863 UT under a hazy sky. The spectra of the object show prominent emission lines in H-alpha, H-beta, and O I (777.4 nm) on a highly reddened continuum. These features suggest that the object is a classical nova past maximum light, highly reddened by interstellar mediums. A spectrum is posted at website URL http://www.cc.kyoto-su.ac.jp/~kao/blog/index.php/view/38.