SIMBAD references

Ulisse Munari, Istituto Nazionale di Astrofisica, Padova Astronomical Observatory, observed PNV J17522579-2126215 with the 1.22-m Asiago telescope (operated by the Department of Physics and Astronomy of the University of Padova) on June 28.95 UT (presumed), at a dispersion on 0.231 micron/pixel over the wavelength range 330-770 nm. The spectrum is that of a nova of the He/N type, with hydrogen Balmer and He I in strong emission. The FWHM of the emission lines is 4500 km/s. The object appears to be heavily reddened, with strong interstellar Na I lines visible in absorption.