Why C-12O-16 profiles in dark clouds do not have flat tops

Details Why C-12O-16 profiles in dark clouds do not have flat tops Why C-12O-16 profiles in dark clouds do not have flat tops

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974apj...193l..93m&link_type=abstract

Astrophysical Journal, vol. 193, Oct. 15, 1974, pt. 2, p. L93-L96.

Astronomy and Astrophysics

Astrophysics

9

Brightness Temperature, Carbon Monoxide, Cosmic Dust, Interstellar Gas, Line Shape, Transition Temperature, Carbon 12, Extremely High Frequencies, Line Spectra, Optical Thickness, Oxygen Isotopes, Particle Density (Concentration), Radial Velocity

Scientific paper

Attention is given to variations of the derived values of the excitation temperature of the C-12O-16 lines with radial velocity. The radiative trapping theory presented by Scoville and Solomon (1974) appears to explain the lack of flat-topped C-12O-16 profiles qualitatively. Reasons for quantitative discrepances are briefly examined, giving attention also to the tendency of the C-13O-16 profiles to have flat tops.

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