Accurate F values of astrophysical interest for neutral carbon

Details Accurate F values of astrophysical interest for neutral carbon Accurate F values of astrophysical interest for neutral carbon

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as...99..179h&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 99, no. 1, p. 179-204.

Astronomy and Astrophysics

Astrophysics

66

Carbon, Interstellar Matter, Transition Probabilities, Molecular Interactions, Molecular Orbitals, Oscillator Strengths, Wave Functions

Scientific paper

A new set of accurate transition probabilities based on configuration interaction wavefunctions has been obtained for many transitions of astrophysical interest in the singlet and in the triplet systems and for intercombination lines of C I. The CIV3 code of Hibbert (1980) was used for the calculations and small empirical adjustments were introduced to the diagonal matrix elements in order to reproduce accurately the observed energy splittings between the energy states. The accuracy of the results has been tested from comparisons with the experimental and theoretical results previously available.

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