Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26a...420..775a&link_type=abstract
Astronomy and Astrophysics, v.420, p.775-781 (2004)
Astronomy and Astrophysics
Astrophysics
25
Atomic Data, Atomic Processes, Plasmas
Scientific paper
We have calculated dielectronic recombination rate coefficients for 22 ions of the boron isoelectronic sequence, between C+ and Xe49+, within the generalized collisional-radiative framework, as outlined by Badnell et al. (\cite{Badnell2003}). Calculations have been performed from both ground and metastable initial states, in both LS- and intermediate-coupling, allowing for Δ n=0 and Δ n=1 core-excitations. Results are presented and discussed for a selection of ions from the sequence. Results which are not presented here can be accessed from the Atomic Data and Analysis Structure (ADAS) database (Summers \cite{Summers2003}) or from the Oak Ridge Controlled Fusion Atomic Data Center (http://www-cfadc.phy.ornl.gov). Comparison is made with the results of other existing theoretical calculations.
Altun Zikri
Badnell Nigel R.
Colgan James
Pindzola M. S.
Yumak A.
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