SIMBAD references

D. K. Lynch, R. W. Russell, R. J. Rudy, and T. Prater, The Aerospace Corporation; and C. E. Woodward, University of Minnesota, report 0.8- to 5.5-micron spectroscopy of V390 Nor (cf. IAUC 8850) using the Infrared Telescope Facility's 3-m telescope (+ SpeX) on June 21 UT. V390 Nor is confirmed as a classical nova well into its emission-line phase. While the spectrum is dominated by low- excitation lines of H I, C I, N I, O I, and Ca II, He I features are already evident. Fe II emission is present but is not strong. Weak P-Cyg profiles extending to 1800 km/s from line center are present on the H I, He I, and O I lines and on the very strong Ca II infrared triplet. The reddening derived from the strong O I lines is E(B-V) approximately 1.0, and there is no evidence of dust in the nova shell.