LAUSR

The intrinsic intensity (band strength) of the fundamental vibrational band of crystalline carbon monoxide (CO) was first determined 50 years ago, but those pioneering measurements have seldom been revisited despite CO's importance in interstellar and Solar System chemistry and CO's abundance and distribution in extraterrestrial environments. On the semi-centennial of those first measurements, which remain in wide use among observational and laboratory astrochemists, we have reexamined those infrared (IR) band-strength determinations, including the density and refractive index data on which they rest, and find that the published results rest on a mere two data points. Here we use new laboratory data to identify and address errors and concerns in that original work from a half-century ago, plus a result from nearly 100 years ago. We report new IR intensities for crystalline CO's fundamental IR band over a range of temperatures and resolutions for the first time, finding that there is not a single unique band strength that applies to all conditions. Optical constants have been calculated, including a set at a higher resolution than in the literature. We also present the first direct IR intensity measurements of the fundamentals of solid 13C16O, 12C17O, and 12C18O. Finally, the first IR transmission spectrum of amorphous CO is presented along with a band-strength estimate. All results are for temperatures below 30 K, and so are relevant to studies of solid CO in the outer Solar System and the interstellar medium.