SIMBAD references

L. Kiss and A. Jacob, University of Sydney, report: "Optical spectra (0.05 nm/pixel, ranges 350-450 and 610-700 nm) were obtained during the rebrightening of this nova on May 12.66 and 13.67 UT with the Siding Spring 2.3-m telescope (+ DBS CCD spectrograph). The Balmer hydrogen series of emission lines shows complex multiple P-Cyg profiles. The H_alpha emission component has a 1600 km/s FWHM, while four distinct absorption components can be identified at -900, -1300, -1600, and -1800 km/s. The H_gamma, H_delta, and H_epsilon lines have similar profiles, with comparably strong Fe II emission lines at 417.6 and 423.3 nm, also with P-Cyg profiles."