Issue |
A&A
Volume 421, Number 3, July III 2004
|
|
---|---|---|
Page(s) | 1185 - 1191 | |
Section | Atomic, molecular, and nuclear data | |
DOI | https://doi.org/10.1051/0004-6361:20040380 | |
Published online | 29 June 2004 |
Experimental Mg IX photorecombination rate coefficient
1
Institut für Atom- und Molekülphysik, Justus-Liebig-Universität Giessen, Leihgesterner Weg 217, 35392 Giessen, Germany
2
Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany
Corresponding author: S. Schippers, Stefan.E.Schippers@strz.uni-giessen.de
Received:
3
March
2004
Accepted:
2
April
2004
The rate coefficient for radiative and dielectronic
recombination of beryllium-like magnesium ions was measured with
high resolution at the Heidelberg heavy-ion storage ring TSR. In
the electron-ion collision energy range 0–207 eV resonances due
to (
) and
(
)
core excitations were detected. At low energies below 0.15 eV the
recombination rate coefficient is dominated by strong
resonances with the strongest one
occuring at an energy of only 21 meV. These resonances decisively
influence the
recombination rate coefficient in a low
temperature plasma. The experimentally derived
dielectronic recombination rate coefficient (±
systematical uncertainty) is compared with the recommendation by
Mazzotta et al. (1998, A&AS, 133, 403) and the recent
calculations by Gu (2003, ApJ, 590, 1131) and by Colgan et al. (2003, A&A, 412, 597). These results deviate from the experimental rate coefficient by 130%, 82% and 25%,
respectively, at the temperature where the fractional abundance of
is expected to peak in a photoionized plasma. At this temperature a theoretical uncertainty in the
resonance positions of only 100 meV
would translate into an uncertainty of the plasma rate coefficient
of almost a factor 3. This finding emphasizes that an accurate
theoretical calculation of the
recombination rate
coefficient from first principles is challenging.
Key words: atomic data / atomic processes / line: formation / plasmas / radiation mechanisms: general
© ESO, 2004
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