SIMBAD references

A. Arai, M. Nagashima, T. Kajikawa, and C. Naka, Koyama Astronomical Observatory (KAO), Kyoto Sangyo University, report that low-resolution (R about 550) spectra of PNV J18102135-2305306 were obtained at the KAO on Mar. 28.725 UT under a hazy sky. The spectra show prominent emission lines of H_alpha, H_beta, and Fe II (multiplets 42, 48, 49) on a highly reddened continuum. The FWHM of the H_alpha emission line is about 900 km/s, and the Na D absorption line is also seen (equivalent width about 0.7 nm). These features suggest that the object is a classical nova that is reddened by interstellar matter.