Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apjs..108..389m&link_type=abstract
Astrophysical Journal Supplement v.108, p.389
Astronomy and Astrophysics
Astronomy
18
Atomic Data, Relativity
Scientific paper
The R-matrix method is used to calculate collision strengths from ground state to the first 26 fine-structure levels of Fe XVII by including the relativistic term coupling coefficients in the semi--Breit-Pauli approximation. Configuration interaction wave functions are used to represent the 15 lowest LS-coupled target states in the R-matrix expansion. Results obtained are compared with the other distorted wave calculations.
Eissner Werner
Mohan Man
Sharma Rinku
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