SIMBAD references

R. J. Rudy, D. K. Lynch, C. C. Venturini, S. Mazuk, D. Broadwater, and M. Cowan, The 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 V2575 Oph (cf. IAUC 8671, 8710) on June 14.34 UT using the VNIRIS spectrograph on the Lick 3-m telescope. The nova shows strong H I and very strong He I emission with He II weakly present. The object is heavily reddened, with E(B-V) = 1.5 as deduced from the O I lines. [O I] and [N II] emission lines are present at the optical wavelengths. The permitted emission lines display broad, doubled profiles with FHWM about 1700 km/s. The profiles of the forbidden lines are narrower (1100 km/s) and are not doubled. There is no evidence for emission from dust. The following magnitudes for V2575 Oph were determined from the spectroscopy: V = 15.3, J = 10.7, H = 11.0, K = 10.1.