Structure of rotational levels and mechanisms of interstellar molecule CH excitation

Details Structure of rotational levels and mechanisms of interstellar molecule CH excitation Structure of rotational levels and mechanisms of interstellar molecule CH excitation

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7625117b&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Hyperfine Structure, Molecular Energy Levels, Molecular Excitation, Molecular Rotation, Galactic Radio Waves, Hydrocarbons, Infrared Radiation, Interstellar Matter, Molecular Structure, Radio Sources (Astronomy), Transition Probabilities

Scientific paper

The peculiarities of the structure of rotational level of the CH-molecule detected in H I and H II galactic region radio-frequency emission, as well as its mechanisms of excitation, are dealt with. It is shown that in the 2 Pi 1/2 CH state, the anomalous variation of Kronig symmetry takes place in transition from rotational lambda-doublet J 1/2 to lambda-doublet J 3/2. The hyperfine constants and lambda-doubling constants are determined. Mechanisms of rotational sublevel excitation are discussed and observational results presented.

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