SIMBAD references

D. K. Lynch, R. J. Rudy, S. Mazuk, and C. C. Venturini, Aerospace Corporation; R. C. Puetter, University of California at San Diego; and R. B. Perry, Langley Research Center, NASA, report 0.4-2.5-micron spectroscopy of V5114 Sgr on June 22.4 UT using the enhanced Aerospace NIRIS spectrograph on the Lick Observatory 3-m telescope. The nova is well into its coronal phase, showing lines of [S VIII] 0.9911-micron, [Si IX] 1.2517-microns, and [Si VI] 1.9641-microns. [Ca VIII] 2.3205-microns was not seen. The Lyman-beta-fluoresced O I lines at 1.1287 and 0.8446 microns were strong. Also present were the unidentified novae lines at 1.1114, 1.1900, 1.5545, and 2.0996 microns. Balmer, Paschen, and Bracket lines are evident, and He I 1.0830-microns is the strongest line in the spectrum. The lines were flat-topped or slightly doubled, indicating spherical or nearly spherical expansion with FWHM approximately 2200 km/s.