Abstract
Effective collision strengths for electron-impact excitation of the N-like ion S x are calculated in the close-coupling approximation using the multichannel R-matrix method. Specific attention is given to the 10 astrophysically important fine-structure forbidden transitions among the 4SO, 2Do and 2Po levels in the 2s22p3 ground configuration. The total (e- + ion) wavefunction is expanded in terms of the 11 lowest LS eigenstates of S x, and each eigenstate is represented by extensive configuration-interaction wavefunctions. The collision strengths obtained are thermally averaged over a Maxwellian distribution of velocities, for all 10 fine-structure transitions, over the range of electron temperatures log T(K) = 4.6-6.7 (the range appropriate for astrophysical applications). The present effective collision strengths are the only results currently available for these fine-structure transition rates.
| Original language | English |
|---|---|
| Pages (from-to) | 677-682 |
| Number of pages | 6 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 308 |
| Issue number | 3 |
| Publication status | Published - 21 Sept 1999 |
Keywords
- Atomic processes
- Line: formation
ASJC Scopus subject areas
- Space and Planetary Science
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