| Issue |
Astron. Astrophys. Suppl. Ser.
Volume 142, Number 1, February II 2000
|
|
|---|---|---|
| Page(s) | 85 - 94 | |
| DOI | https://doi.org/10.1051/aas:2000139 | |
| Published online | 15 February 2000 | |
Recombination coefficients for CII lines*
1
Department of Physics, Montana State University, Bozeman, MT 59717-3840, U.S.A.
2
Department of Physics and Astronomy, University College London, Gower St., London, WC1E 6BT, UK e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
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Send offprint request to: P.J. Storey
Received:
20
July
1999
Accepted:
4
October
1999
Abstract
Effective recombination coefficients are given for CII transitions
between doublet states. The calculations are carried out in the temperature
range
and for an electron density of
104 cm-3. The effects of electron collisions on the excited states
are included. The necessary bound-bound and bound-free radiative data are
obtained from a new R-matrix calculation in which photoionization resonances
are fully delineated, thereby accurately incorporating the effects of both
radiative and dielectronic recombination. The R-matrix calculation includes
all bound states with principal quantum number
and total orbital
angular momentum
. The effect of moving the resonance features to
their experimentally determined positions is also investigated and found to
be important at low temperatures.
Key words: atomic data / line: formation / HII regions / planetary nebulae: general
Tables 1–5 are also available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html
© European Southern Observatory (ESO), 2000
