SIMBAD references

R. W. Russell, D. K. Lynch, and R. J. Rudy, The Aerospace Corporation, report 0.8-2.5-micron spectroscopy of V5116 Sgr on July 15 UT using SpeX at the Infrared Telescope Facility. The nova showed emission lines of H I, He I, C I, N I, Ca II, and O I with FWHM about 2200 km/s. P-Cyg profiles were observed on the He I lines at 1.0830 and 2.0581 microns. There was no evidence of thermal emission from dust.