High-resolution absorption cross sections of carbon monoxide bands at 295 K between 91.7 and 100.4 nanometers

Details High-resolution absorption cross sections of carbon monoxide bands at 295 K between 91.7 and 100.4 nanometers High-resolution absorption cross sections of carbon monoxide bands at 295 K between 91.7 and 100.4 nanometers

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...369..574s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 369, March 10, 1991, p. 574-580. Research supported by the Japanese Society

Astronomy and Astrophysics

Astrophysics

48

Absorption Cross Sections, Carbon Monoxide, Interstellar Matter, Ultraviolet Spectra, Far Ultraviolet Radiation, High Resolution, Hydrogen, Photoabsorption, Spectral Bands, Synchrotron Radiation

Scientific paper

Theoretical descriptions of the abundance and excitation of carbon monoxide in interstellar clouds require accurate data on the vacuum-ultraviolet absorption spectrum of the molecule. The 6.65 m spectrometer at the Photon Factory synchrotron light source was used to measure photoabsorption cross sections of CO features between 91.2 and 100.4 nm. These data were recorded at a resolving power of 170,000, more than 20 times greater than that used in previous work.

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