Bound-bound radiative transitions in C I

Details Bound-bound radiative transitions in C I Bound-bound radiative transitions in C I

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...140..383n&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 140, no. 2, Nov. 1984, p. 383-389.

Astronomy and Astrophysics

Astrophysics

51

Absorption Spectra, Comets, Interstellar Matter, Transition Probabilities, Carbon, Electron Transitions, Line Spectra, Oscillator Strengths, Spin-Orbit Interactions, Tables (Data)

Scientific paper

For the six energetically lowest configurations of C0, radiative transition probabilities are calculated by two different methods. For the prominent interstellar C I multiplets longwards of 1260 Å, the authors find considerable differences against oscillator strengths derived from astronomical observations. They further investigate a radiative excitation process for the cometary C I λ1931 emission.

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