SIMBAD references

Akira Arai and Mizuki Isogai, Koyama Astronomical Observatory (KAO), Kyoto Sangyo University, report that they obtained low-resolution (R about 550) spectrograms of PNV J17260708-2551454 with the 1.3-m Araki telescope at KAO on Mar. 27.74 UT. The spectra show prominent emission in H_alpha with P-Cyg profiles on a highly reddened continuum. H_beta, Fe II, and O I 777.4-nm are also visible. The FWHM of the H_alpha emission is about 600 km/s. These features suggest that the object is an "Fe II-type" classical nova. The spectra are posted at the following website URL: http://www.cc.kyoto-su.ac.jp/~kao/blog/index.php/view/165.