Oscillator strengths and predissociation rates for Rydberg transitions in 12C16O, 13C16O, and 13C18O involving the E1II, B 1Σ+ and W 1II states

One of the processes controlling the interstellar CO abundance and the ratio of its isotopologues is photodissociation. Accurate oscillator strengths and predissociation rates for Rydberg transitions are needed for modeling this process. We present results on absorption from the E-1 Pi-X-1 Sigma(+) (1-0) and B-1 Sigma(+)-X-1 Sigma(+) (6-0) bands at 1051 and 1002 angstrom, respectively, and the vibrational progression E-1 Pi-X-1 Sigma(+) (v'-0) bands with v(') = 0-3 at 972, 956, 941, and 925 angstrom, respectively. The corresponding spectra were acquired at the high resolution (R approximate to 30; 000) SU5 beam line at the Super ACO Synchrotron in Orsay, France. Spectra were obtained for the (CO)-C-12-O-16, (CO)-C-13-O-16, and (CO)-C-13-O-18 isotopologues. These represent the most complete set of measurements available. Comparison is made with earlier results, both empirical and theoretical. While earlier determinations of oscillator strengths based on absorption from synchrotron radiation tend to be somewhat smaller than ours, the suite of measurements from a variety of techniques agree for the most part, considering the mutual uncertainties. For the bands studied here, their relative weakness, or their significant line widths arising from predissociation, minimizes potential problems from large optical depths at line center in absorption measurements. Predissociating line widths could generally be extracted from the spectra thanks to the profile simulations used in the analysis. In many cases, these simulations allowed us to consider e and f parity levels separately and to determine the dependence of the width on rotational quantum number, J. Our results are consistent with earlier determinations, especially the widths inferred from laser experiments.