SIMBAD references

A. Evans, Keele University; T. Kerr, Joint Astronomy Centre; Y. Matsuoka and Y. Tsuzuki, University of Tokyo; T. R. Geballe, Gemini Observatory; R. D. Gehrz and C. E. Woodward, University of Minnesota; M. F. Bode, Liverpool John Moores University; T. J. O'Brien and R. J. Davis, University of Manchester; J. P. Osborne and K. L. Page, University of Leicester; G. Schwarz, West Chester University; S. Starrfield and J.-U. Ness, Arizona State University; J. Krautter, University of Heidelberg; J. Drake, Smithsonian Astrophysical Observatory; and S. P. S. Eyres, University of Central Lancashire, report that a spectrum (range 880 nm-2.5 microns) was obtained with the 3.8-m U.K. Infrared Telescope (+ UIST) on Feb. 24.64 UT. The spectra show strong Paschen lines from 4-3 to 12-3, Brackett lines from 7-4 to 20-4, Pfund lines from 17-5 to 23-5, He I at 1.083, 2.058, and 2.112 microns, O I 3P-3D**0 at 1.128 microns (cf. IAUC 8673), and other lines that are tentatively identified with O I, O II and C I. The FWHM of the resolved Paschen_alpha line is 1130 ± 50 km/s, but with wings extending to 3000 km/s.