SIMBAD references

Kazuya Ayani, Bisei Astronomical Observatory, reports that M. Fujii (Kurashiki, Okayama, Japan) obtained a spectrogram of PNV J18523496-0018423 on Oct. 21.419 UT with 0.4-m telescope at the Fujii Kurosaki Observatory and found that its H-alpha emission had a P-Cyg profile; the difference between the absorption bottom and the emission peak being about 500 km/s. He also found a Na I D absorption line whose equivalent width is about 0.6 nm, noting also that the slope of the continuum indicates heavy interstellar reddening. His spectrum is posted at the following website URL: http://otobs.org/FBO/etc/pnv_j18523496-0018423_20121021.gif.