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: rk@star.ucl.ac.uk, pjs@star.ucl.ac.uk
Send offprint request to: P.J. Storey
Received:
20
July
1999
Accepted:
4
October
1999
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
© European Southern Observatory (ESO), 2000