SIMBAD references

D. K. Lynch, R. W. Russell, and R. J. Rudy, The Aerospace Corporation; M. Sitko, Space Science Institute; and C. E. Woodward, University of Minnesota, report 0.8- to 5.5-micron spectroscopy of the nova V2468 Cyg (cf. IAUC 8927, 8928, 8936) on Oct. 4 UT using the Infrared Telescope Facility (+ Spex). Though V2468 Cyg had faded by more than a factor of two since mid-August, the coronal lines have strengthened significantly. The [Si VI] line at 1.96 microns is among the strongest of the emission features. Lines of [S VIII], [S IX], [Al IX], and [Ca VIII] are also present. Several Rydberg lines are present, including those at 0.89, 1.19, 1.11, 1.55, and 2.1 microns.