SIMBAD references

N. M. Ashok and D. P. K. Banerjee, Physical Research Laboratory, Ahmedabad, report that near-infrared JHK spectroscopy (range 1.08-2.35 microns) of V574 Pup, taken on Nov. 26.98 UT with the Mt. Abu 1.2-m telescope (+ PRL Near-Infrared Imaging Spectrometer), shows strong H I emission lines of Paschen_beta, Paschen_gamma, Brackett_gamma, and Brackett 11 to 17. Prominent O I lines at 1.1288 and 1.3166 microns are seen, as are a blend of N I and C I lines in the region around 1.175 and 1.25 microns.