Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000apj...544..575t&link_type=abstract
The Astrophysical Journal, Volume 544, Issue 1, pp. 575-580.
Astronomy and Astrophysics
Astronomy
10
Atomic Data
Scientific paper
Electron excitation collision strengths for fine-structure transitions in Fe X, Fe XI, and Fe XIII are calculated using full Breit-Pauli R-matrix approach. We included 49 fine-structure levels of Fe X, 38 fine-structure levels of Fe XI, and 26 fine-structure levels of Fe XIII in our scattering calculations. These levels are represented by configuration-interaction wave functions. The relativistic effects are included in the Breit-Pauli approximation via one-body mass correction, Darwin, and spin-orbit interaction terms in the scattering equations. Rydberg series of resonances converging to the excited state thresholds are explicitly included in the calculations. The effective collision strengths are determined by integrating collision strengths and assuming a Maxwellian distribution of electron energies.
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