Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001mnras.325..159w&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 325, Issue 1, pp. 159-166.
Astronomy and Astrophysics
Astronomy
2
Atomic Processes, Line: Formation
Scientific paper
The ab initio R-matrix method is used to calculate effective collision strengths for electron-impact excitation of the phosphorous-like ion Kv in the close-coupling approximation. All 10 astrophysically important fine-structure forbidden transitions within the 3s23p3 4S3/2o, 2D3/2,5/2o, 2P1/2,3/2o ground configuration levels are considered. The 22 lowest LSQ2 target states are included in the calculation. Effective collision strengths are obtained by averaging the electron collision strengths over a Maxwellian distribution of electron velocities. Results are presented for electron temperatures in the range logT(K)=3.3 to logT(K)=5.1, appropriate for astrophysical applications. Comparisons are made with previous work and significant discrepancies are noted. We believe that the results are the most accurate to date.
Bell Kenneth L.
Wilson J. N.
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