SIMBAD references

D. K. Lynch, R. J. Rudy, C. C. Venturini, and S. Mazuk, Aerospace Corporation; R. C. Puetter, University of California at San Diego; and R. B. Perry, Langley Research Center, NASA, report 0.47- to 2.5-micron spectroscopy of V2576 Oph (cf. IAUC 8700, 8710) on June 14.4 UT using the VNIRIS spectrograph on the Lick 3-m telescope. This Fe II nova has broad (2700 km/s), flat-topped emission lines. There is very little reddening [E(B-V) = 0.25] and no evidence of dust in the nova ejecta. The object displays weak coronal lines from [S VIII] and [Si VI], and the unidentified features at 1.11, 1.19, 1.55, and 2.10 microns are present. Magnitudes for V2576 Oph: V = 13.9, J = 11.2, H = 11.7, K = 11.0.