SIMBAD references

R. W. Russell, D. K. Lynch, R. J. Rudy, The Aerospace Corporation; and C. E. Woodward, University of Minnesota, report on IRTF SpeX observations, obtained as above on Apr. 12.62 UT: "V459 Vul is one of the small number of classical novae to display C I and coronal lines simultaneously. Of the latter, [S IX] at 1.25 microns is the highest-excitation and [Si VI] at 1.96 microns is the strongest. He II lines and the unidentified novae lines are present as well. The O I lines, which are still quite strong, indicate a reddening of E(B-V) = 1.0, some of which is probably local to the nova since the spectrum exhibits thermal emission from dust beyond 1.5 microns."