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High-resolution spectra and photoabsorption coefficients for carbon monoxide absorption bands between 94.0 nm and 100.4 nmPhotoabsorption 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.
Document ID
19900027125
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Yoshino, K.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Stark, G.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Smith, P. L.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Parkinson, W. H.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Ito, K.
(National Laboratory for High Energy Physics Oho, Japan)
Date Acquired
August 14, 2013
Publication Date
March 1, 1988
Publication Information
Publication: Supplement
Volume: 49
ISSN: 0449-1947
Subject Category
Astrophysics
Accession Number
90A14180
Funding Number(s)
CONTRACT_GRANT: NSG-7304
Distribution Limits
Public
Copyright
Other

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