Dielectronic recombination data for astrophysical applications: Plasma rate-coefficients for Fe^q+ (q=7-10, 13-22) and Ni^25+ ions from storage-ring experiments

Abstract

This review summarizes the present status of an ongoing experimental effort to provide reliable rate coefficients for dielectronic recombination of highly charged iron ions for the modeling of astrophysical and other plasmas. The experimental work has been carried out over more than a decade at the heavy-ion storage-ring TSR of the Max-Planck-Institute for Nuclear Physics in Heidelberg, Germany. The experimental and data reduction procedures are outlined. The role of previously disregarded processes such as fine-structure core excitations and trielectronic recombination is highlighted. Plasma rate coefficients for dielectronic recombination of Fe${}^{q+}$ ions (q=7-10, 13-22) and Ni${}^{25+}$ are presented graphically and in a simple parameterized form allowing for easy use in plasma modeling codes. It is concluded that storage-ring experiments are presently the only source for reliable low-temperature dielectronic recombination rate-coefficients of complex ions.

This replacement corrects the coefficients for q=15 in the last column of Table II and Figure 7 accordingly. The previous coefficients were other than stated for 3->3 DR only. The present coefficients comprise 3->3 and 3->4 DR as stated and reproduce the Fe15+ DR plasma rate coefficient from Figure 7 of Ref. 5. We thank Houke Huang (IMP, Lanzhou, China) for pointing out the error