Conference paper
Authors list: Schippers, S.; Böhm, S.; Müller, A.; Gwinner, G.; Schnell, M.; Schwalm, D.; Wolf, A.; Savin, D.W.
Appeared in: Stellar coronae in the chandra and XMM-Newton era
Editor list: Favata, Fabio; Drake, Jeremy J.
Publication year: 2002
Pages: 591-595
ISBN: 1-58381-119-2
eISBN: 978-1-58381-612-7
Conference: Conference "Stellar Coronae in the Chandra and XMM-Newton Era"
Title of series: Astronomical Society of the Pacific conference series
Number in series: 277
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 Civ 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.
Abstract:
Citation Styles
Harvard Citation style: Schippers, S., Böhm, S., Müller, A., Gwinner, G., Schnell, M., Schwalm, D., et al. (2002) Recombination rate coefficients for astrophysical applications from storage-ring experiments, in Favata, F. and Drake, J. (eds.) Stellar coronae in the chandra and XMM-Newton era. San Francisco, Calif.: Astronomical Society of the Pacific. pp. 591-595
APA Citation style: Schippers, S., Böhm, S., Müller, A., Gwinner, G., Schnell, M., Schwalm, D., Wolf, A., & Savin, D. (2002). Recombination rate coefficients for astrophysical applications from storage-ring experiments. In Favata, F., & Drake, J. (Eds.), Stellar coronae in the chandra and XMM-Newton era. (pp. 591-595). Astronomical Society of the Pacific.
