SIMBAD references

D. Balam, Dominion Astrophysical Observatory, National Research Council of Canada (NRCC); and G. Sarty, University of Saskatchewan, write that a spectrogram (range 429-455 nm, resolution 0.02 nm), obtained with the NRCC 1.82-m Plaskett telescope on Nov. 10.08 UT, confirms that this object is a nova, showing H_alpha emission (HWZI about 400 km/s) with a P-Cyg profile, its absorption minimum being blue-shifted by 700 km/s with respect to the emission peak. Additional lines showing P-Cyg profiles include N II (448.1 nm), Fe II (multiplet 27) at 435.0 and 441.8 nm, and Fe II (multiplet 38) at 452.1 nm.