SIMBAD references

L. Kiss, University of Sydney; and K. Sarneczky, University of Szeged, report that optical spectra (0.05 nm/pixel; ranges 400-500 and 580-680 nm) were obtained of N Vul 2007 (cf. IAUC 8861, 8862) on Aug. 18.55 UT with the Siding Spring 2.3-m telescope (+ DBS CCD spectrograph). The spectrum is dominated by strong and flat-topped hydrogen Balmer lines with FWZI approximately 4000-4500 km/s and FWHM approximately 3000 km/s. Similar line profiles are seen in the He I lines at 587.6 and 667.8 nm and the Fe II (27, 28) doublet at 417.8 and 423.3 nm. The strong Na I D absorption lines suggest high interstellar extinction.