Issue |
A&A
Volume 469, Number 3, July III 2007
|
|
---|---|---|
Page(s) | 1203 - 1209 | |
Section | Atomic, molecular, and nuclear data | |
DOI | https://doi.org/10.1051/0004-6361:20077262 | |
Published online | 02 May 2007 |
Atomic data from the IRON project*
LXIV. Radiative transition rates and collision strengths for Ca II
1
Institute for Astrophysics and Computational Sciences, Department of Physics, The Catholic University of America, Washington, DC 20064, USA
2
Exploration of the Universe Division, Code 667, NASA's Goddard Space Flight Center, Greenbelt, MD 20771, USA
3
Centro de Física, Instituto Venezolano de Investigaciones Científicas (IVIC), PO Box 21827, Caracas 1020A, Venezuela e-mail: bautista@kant.ivic.ve
4
Department of Physics, University of Strathclyde, Glasgow G4 0NG, UK
Received:
8
February
2007
Accepted:
19
April
2007
Aims.This work reports radiative transition
rates and electron impact excitation rate coefficients for levels of the
n = 3, 4, 5, 6, 7, 8 configurations of .
Methods.The radiative data were computed using the Thomas-Fermi-Dirac central potential method in the frozen core approximation and includes the polarization interaction between the valence electron and the core using a model potential. This method allows for configuration interactions (CI) and relativistic effects in the Breit-Pauli formalism. Collision strengths in LS-coupling were calculated in the close coupling approximation with the R-matrix method. Then, fine structure collision strengths were obtained by means of the intermediate-coupling frame transformation (ICFT) method which accounts for spin-orbit coupling effects.
Results. We present extensive comparisons with the most recent calculations
and measurements for as well as a comparison between the core polarization results and the
“unpolarized” values.
We find that core polarization affects the computed lifetimes
by up to 20%. Our results are in very close agreement with recent measurements for the
lifetimes of
metastable levels.
The present collision strengths were integrated over
a Maxwellian distribution of electron
energies and the resulting effective collision strengths are given for a
wide range of temperatures.
Our effective collision
strengths for the resonance transitions are within ~11% from
previous values derived from experimental measurements, but disagree with
later computations using the distorted wave approximation.
Key words: atomic data / atomic processes / line: formation
© ESO, 2007
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