Konferenzpaper

Erschienen in: Stellar coronae in the chandra and XMM-Newton era

Herausgeberliste: Favata, Fabio; Drake, Jeremy J.

Jahr der Veröffentlichung: 2002

Seiten: 591-595

ISBN: 1-58381-119-2

eISBN: 978-1-58381-612-7

Konferenz: Conference "Stellar Coronae in the Chandra and XMM-Newton Era"

Serientitel: Astronomical Society of the Pacific conference series

Serienzählung: 277

Abstract: 

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.

Harvard-Zitierstil: 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-Zitierstil: 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.