SIMBAD references

Kazuyoshi Imamura, Okayama University of Science (OUS), reports on obtaining a low-resolution spectrum (R about 400) of PNV J17522579-2126215 on June 28.593 UT, using the DSS-7 spectrometer attached to the 0.28-m Schmidt-Cassegrain telescope at the OUS observatory. Broad and prominent emission lines of the Balmer series, He I (706.5-nm), O I (777.3-nm), and Mg II (788.0-nm) can be seen in the spectrum. The Balmer lines show asymmetrical profiles; the FWHM of H-alpha is approximately 4100 km/s. From this result, the variable is thought to be a classical nova with a large expansion velocity. The spectrum has been posted at the following website URL: http://blog-imgs-44.fc2.com/t/n/b/tnblab/pnSGR_20120628.png.