High-resolution spectra and photoabsorption coefficients for carbon monoxide absorption bands between 94.0 NM and 100.4 NM

Details High-resolution spectra and photoabsorption coefficients for carbon monoxide absorption bands between 94.0 NM and 100.4 NM High-resolution spectra and photoabsorption coefficients for carbon monoxide absorption bands between 94.0 NM and 100.4 NM

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jphys..49...37y&link_type=abstract

(IAU, ESA, CNRS, et al., Colloquium on UV and X-ray Spectroscopy of Astrophysical and Laboratory Plasmas, 102nd, Beaulieu-sur-Me

Astronomy and Astrophysics

Astrophysics

10

Absorption Cross Sections, Carbon Monoxide, Far Ultraviolet Radiation, Interstellar Gas, Photoabsorption, Abundance, High Resolution, Photodissociation, Ultraviolet Spectrometers

Scientific paper

Photoabsorption coefficients have been measured for the CO in interstellar clouds at a resolving power more than 20 times greater than previously obtainable. In order to facilitate comparisons, these data have been integrated over the same wavelength ranges as used in Letzelter et al. (1987). It is found that most of the results obtained for bands between 94.0 and 100.4 nm are larger than those of Letzelter; the discrepancy may be attributable to the difference between the resolving powers of the spectrometers used, because the saturation effects associated with low resolution can underestimate absorption coefficient values.

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