SIMBAD references

S. Mazuk, R. J. Rudy, D. K. Lynch, and C. C. Venturini, 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 V2362 Cyg (cf. IAUC 8698, 8702, 8710) on June 14.6 UT using the VNIRIS spectrograph on the Lick 3-m telescope. The nova is still of low excitation, showing the signature Fe II lines as well as emission of C I, N I, and O I. He I emission lines remain comparatively weak. The reddening determined from the fluorescently excited O I lines is E(B-V) = 0.6; O I 777.4-nm is also present and displays a weak P-Cyg profile. The optical spectrum displays forbidden lines of [O I], [O II], and [N II]. FWHM of the lines was 1500 km/s. There is no evidence of dust in the nova ejecta. Magnitudes for V2362 Cyg: V = 12.4, J = 10.0, H = 10.1, K = 9.5.