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Population Inversion and Suprathermal Excitation in Carbon Monoxide

Published online by Cambridge University Press:  14 August 2015

J. Köppen
Affiliation:
Institut für Theoretische Astrophysik Universität Heidelberg, Germany
W. H. Kegel
Affiliation:
Institut für Theoretische Astrophysik Universität Heidelberg, Germany

Extract

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We have investigated under which physical conditions (kinetic temperature, H2 density, CO column density) the CO molecule shows suprathermal excitation and population inversion. The computations are based on a model in which the excitation is basically due to collisions with H2 molecules. The collision cross-sections were taken from Green and Thaddeus (1976). The radiative transport in the molecular lines is treated in an on-the-spot approximation (see e.g. Kegel 1979)

J = S(1 - e) + Ibge

in order to keep the computing time low enough to permit the investigation of a wide range of parameters. Our approximation of the radiative transfer is mathematically equivalent to a formalism involving an escape probability β = e. This escape probability arises from the fact that the radiative transfer in the line wings is neglected.

Type
Research Article
Copyright
Copyright © Reidel 1980 

References

Green, S., Thaddeus, P.: 1976, Astrophys. J. 205, 766.Google Scholar
Kegel, W.H.: 1979, Astron. Astrophys. Suppl. 38, 131.Google Scholar