SIMBAD references

Kazuya Ayani, Bisei Astronomical Observatory, reports that M. Fujii (Kurashiki, Okayama, Japan) obtained a low-resolution spectrogram of PNV J18193700-1907400 on July 18.572 UT with a 40-cm telescope. Fujii notes that the spectrum shows emission lines of H-alpha, H-beta, H-gamma, Fe II (multiplets 37, 42, 74), and He I (587.6 and 667.8 nm), an absorption line of Na I D (equivalent width 0.2 nm), and DIB absorption (628.4 nm, equivalent width 0.33 nm). The H-alpha emission line has a FWHM of 940 km/s. Fujii also notes that this object may have strong interstellar absorption, judging from the slope of the continuum, adding that the variable may be a "Fe II"-type nova. Fujii's spectrum is posted at the following website URL: http://otobs.org/FBO/novae/pnv_j18193700-1907400.htm.