SIMBAD references

Kazuyoshi Imamura and Minako Ogi, Okayama University of Science (OUS), report obtaining a low-resolution spectrogram (R about 400) of PNV J18193700-1907400 on July 18.529 UT, using the DSS-7 spectrometer attached to the 0.28-m Schmidt-Cassegrain telescope at the OUS observatory. The spectrum shows an H-alpha emission line on a reddened continuum. The FWHM of H-alpha is approximately 1000 km/s. From this result, the variable is thought to be a classical nova. The spectrum has been posted at the following website URL: http://tnblab.blog7.fc2.com/blog-entry-321.html.