Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010apj...721.1603o&link_type=abstract
The Astrophysical Journal, Volume 721, Issue 2, pp. 1603-1607 (2010).
Astronomy and Astrophysics
Astronomy
2
Atomic Data, Atomic Processes, Plasmas
Scientific paper
Recombination of Be-like Si10+ over the 0-43 eV electron-ion energy range is measured at the CRYRING electron cooler. In addition to radiative and dielectronic recombination, the recombination spectrum also shows strong contributions from trielectronic recombination. Below 100 meV, several very strong resonances associated with a spin-flip of the excited electron dominate the spectrum and also dominate the recombination in the photoionized plasma. The resonant plasma rate coefficients corrected for the experimental field ionization are in good agreement with calculated results by Gu and with AUTOSTRUCTURE calculations. All other calculations significantly underestimate the plasma rate coefficients at low temperatures.
Böhm S.
Loch S. D.
Orban I.
Schuch Reinhold
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