Recombination rate coefficients for astrophysical applications from storage-ring experiments

Details Recombination rate coefficients for astrophysical applications from storage-ring experiments Recombination rate coefficients for astrophysical applications from storage-ring experiments

2003-01-10

arxiv.org/abs/astro-ph/0301170v3

ASP Conference Series 277 (2002) 591-595

Astronomy and Astrophysics

Astrophysics

5 pages, 3 figures, Workshop on Stellar Coronae in the Chandra and XMM-Newton era, June 2001, Noordwijk, The Netherlands, for

Scientific paper

The basic approach for measuring electron-ion recombination rate coefficients in merged-beams electron-ion collision experiments at heavy-ion storage rings is outlined. As an example experimental results for the low temperature recombination of C IV ions are compared with the recommended theoretical rate coefficient by Mazzotta et al. The latter deviates by factors of up to 5 from the experimental one.

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