Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26a...365..258p&link_type=abstract
Astronomy and Astrophysics, v.365, p.258-265 (2001)
Astronomy and Astrophysics
Astrophysics
12
Atomic Data
Scientific paper
Electron excitation collision strengths for fine-structure transitions 3s23p5-3s3p6, 3s23p5-3s23p43d and 3s3p6-3s23p43d in Fe x, are calculated using a 180-level Breit-Pauli R-matrix calculation containing the above levels together with those from 3s3p53d and 3s23p33d2 configurations. The collision strength is averaged over a Maxwellian velocity distribution to obtain the effective fine-structure collision strengths as a function of electron temperature from log T(K)=5.4-7.0. We show that low-energy resonances enhance the effective collision strength, with significant effects on level populations.
Berrington Keith A.
Pelan J. C.
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