Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26as...46..101g&link_type=abstract
Astronomy and Astrophysics Supplement Series, vol. 46, Oct. 1981, p. 101-103.
Astronomy and Astrophysics
Astrophysics
Atomic Excitations, Carbon, Ions, Isoelectronic Sequence, Valence, Wave Functions, Astrophysics, Born Approximation, Electron Transitions, Ground State, Quasars, Stellar Spectra
Scientific paper
An analytic atomic independent particle model is used to generate wave functions for the valence and excited states of isoelectronic ions of carbon up to Z = 20. Using these wave functions in conjunction with the Born approximation and the Russell-Saunders LS-coupling scheme, f values are calculated for various transitions from the 2p2(3P0) ground state. The results are compared with those from other works.
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