Sc. Tegler et al., DETECTION OF THE 2165 INVERSE CENTIMETER (4.619 MICRON) XCN BAND IN THE SPECTRUM OF L1551 IRS-5, The Astrophysical journal, 411(1), 1993, pp. 260-265
We report the detection of a broad absorption band at 2165 cm-1 (4.619
mum) in the spectrum of L1551 IRS 5. New laboratory results over the
2200-2100 cm-1 wavenumber interval (4.55-4.76 mum), performed with rea
listic interstellar ice analogs, suggest that this feature is due to a
CN-containing compound. We will refer to this compound as XCN. We als
o confirm the presence of frozen CO (both in nonpolar and polar matric
es) through absorption bands at 2140 cm-1 (4.67 mum) and 2135 cm-1 (4.
68 mum). The relative abundance of solid-state CO to frozen H2O is app
roximately 0.13 while the abundance of XCN seems comparable to that of
frozen CO.