SIMBAD references

R. K. Das, N. M. Ashok, and D. P. K. Banerjee, Physical Research Laboratory (PRL), Navrangpura, report that their near- infrared JHK spectroscopy (range 1.08-2.35 microns) of V477 Sct, obtained with the Mt. Abu 1.2-m telescope (+ PRL Near-Infrared NICMOS3 Imaging Spectrometer), on Oct. 15.75 UT, are typical of a classical nova and show prominent H I emission lines of the Paschen and Brackett series. Preliminary estimates for the Paschen-beta H I line indicate a FWZI of 6000 km/s or more. O I lines, generally seen in classical-novae spectra, are also seen with the continuum fluorescence 1.3166-micron line being stronger than the Lyman-beta excited fluorescence O I line at 1.1288 microns.