The population of highly excited levels of carbon atoms

Details The population of highly excited levels of carbon atoms The population of highly excited levels of carbon atoms

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18..215p&link_type=abstract

Soviet Astronomy Letters, Vol. 18, p. 215; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 6, June 1992, p. 541

Astronomy and Astrophysics

Astronomy

10

Atomic Energy Levels, Carbon, Cosmic Plasma, Electron Capture, Fine Structure, Molecular Clouds, Interstellar Matter, Ionization Potentials, Radio Astronomy

Scientific paper

The carbon departure coefficients bn and betan are calculated for typical conditions of molecular clouds. Radiationless electron capture with simultaneous excitation of the fine structure of the core and the collisional stabilization of the highly excited levels that are formed were taken into account. The relative population of the fine structure levels of the core is calculated from the medium's parameters.

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