Electron-ion recombination for $\ion{Fe}{viii}$ forming $\ion{Fe}{vii}$ and $\ion{Fe}{ix}$ forming $\ion{Fe}{viii}$: measurements and theory

The photorecombination rate coefficients of potassium-like $\ion{Fe}{viii}$ ions forming calcium-like $\ion{Fe}{vii}$ and of argon-like $\ion{Fe}{ix}$ forming potassium-like $\ion{Fe}{viii}$ were measured by employing the merged electron-ion beams method at the Heidelberg heavy-ion storage-ring TSR....

Full description

Saved in:
Bibliographic Details
Published inAstronomy and astrophysics (Berlin) Vol. 492; no. 1; pp. 265 - 275
Main Authors Schmidt, E. W., Schippers, S., Bernhardt, D., Müller, A., Hoffmann, J., Lestinsky, M., Orlov, D. A., Wolf, A., Lukić, D. V., Savin, D. W., Badnell, N. R.
Format Journal Article
LanguageEnglish
Published EDP Sciences 01.12.2008
Subjects
Online AccessGet full text

Cover

Loading…
More Information
Summary:The photorecombination rate coefficients of potassium-like $\ion{Fe}{viii}$ ions forming calcium-like $\ion{Fe}{vii}$ and of argon-like $\ion{Fe}{ix}$ forming potassium-like $\ion{Fe}{viii}$ were measured by employing the merged electron-ion beams method at the Heidelberg heavy-ion storage-ring TSR. New theoretical calculations with the AUTOSTRUCTURE code were carried out for dielectronic recombination (DR) and trielectronic recombination (TR) for both ions. We compare these experimental and theoretical results and also compare with previously recommended rate coefficients. The DR and TR resonances were experimentally investigated in the electron-ion collision energy ranges 0–120 eV and 0–151 eV for $\ion{Fe}{viii}$ and $\ion{Fe}{ix}$. Experimentally derived $\ion{Fe}{viii}$ and $\ion{Fe}{ix}$ DR + TR plasma rate coefficients are provided in the temperature range $k_{\rm B}T=0.2$ to $1000~{\rm eV}$. Their uncertainties amount to <$\pm26\%$ and <$\pm35\%$ at a 90% confidence level for $\ion{Fe}{viii}$ and $\ion{Fe}{ix}$, respectively.
Bibliography:publisher-ID:aa10834-08
istex:2FE3563B955361FBA1294E640C7D8F3E47873B10
other:2008A%26A...492..265S
ark:/67375/80W-K35TF622-Z
ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361:200810834