SIMBAD references

D. K. Lynch, R. W. Russell, and R. J. Rudy, Aerospace Corporation, report that spectroscopy (range 0.8-2.5 microns) of V1187 Sco (cf. IAUC 8380, 8382), taken with the Infrared Telescope Facility (+ SpeX) on Apr. 18.7 UT, shows that the object had faded considerably (K = 13.2 from the spectrum) and that the lines were still broad. H I and He I 1.0830- and 2.0581-microns were present (2900 km/s FWHM), as were some weak He II lines. There was a surprising lack of coronal lines, although the [Si VI] 1.9645- micron line was strong and appeared to be split into two strong, well-separated components. The unidentified novae lines at 1.19 and 1.55 microns were present. There was no evidence of thermal emission from dust.