Abstract
Photoionization cross-sections out of the fine-structure levels (2S(2)2p(4) P-3(2,0,1)) of the O-like Fe ion Fe XIX have been reinvestigated. Data for photoionization out of each of these finestructure levels have been obtained, where the calculations have been performed with and without the inclusion of radiation damping on the resonance structure in order to assess the importance of this process. Recombination rate coefficients are determined using the Milne relation, for the case of an electron recombining with N-like Fe ions (Fe XX) in the ground state to form O-like Fe (Fe XIX) existing in each of the fine- structure ground-state levels. Recombination rates are presented over a temperature range similar to 4.0 less than or equal to log T-e less than or equal to 7.0, of importance to the modelling of X-ray emission plasmas.
Original language | English |
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Pages (from-to) | 442-450 |
Number of pages | 9 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 328 |
Issue number | 2 |
Publication status | Published - 01 Dec 2001 |
ASJC Scopus subject areas
- Space and Planetary Science