0.8-2.5 μm Spectroscopy of Novae

摘要

We present new infrared results on a number of recent novae including V2274 Cyg (Nova Cygni 2001), CI Aquilae, and V723 Cas (Nova Cassiopeiae 1995), and review some of the outstanding aspects of their infrared spectra. The discussion includes the identification of coronal lines and their interpretation and structure in the CO emission band at 2.3 μm.