SIMBAD references

H. L. Malasan, J. Suherli, and E. Wiyando, Bosscha Observatory, Institut Teknologi Bandung, Indonesia; and A. Arai and H. Kawakita, Koyama Astronomical Observatory, Kyoto Sangyo University, Japan, report on optical spectroscopic observations (R about 400) of PNV J14542000-5505030 = PR Lup on Aug. 16.6 UT at Bosscha Observatory using a 20-cm Schmidt-Cassegrain telescope (+ SBIG DSS7 spectrograph). The spectra exhibit strong H-alpha, H-beta, and Fe II multiplet emissions, suggesting that the variable is a "Fe II"-type classical nova. P-Cygni profiles are absent, and the FWHM of the H-alpha emission is about 1700 km/s.