Recombination coefficients for C II lines TeX Export

@article{citeulike:6083690, abstract = {Effective recombination coefficients are given for C II transitions between doublet states. The calculations are carried out in the temperature range \$500 - 20\,000\;{K}\$ and for an electron density of 10^4 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 \$n \leq 15\$ and total orbital angular momentum \$L \leq 4\$. The effect of moving the resonance features to their experimentally determined positions is also investigated and found to be important at low temperatures.}, author = {Davey, A. R. and Storey, P. J. and Kisielius, R.}, citeulike-article-id = {6083690}, citeulike-linkout-0 = {http://aas.aanda.org/index.php?option=article&access=standard&Itemid=129&url=/articles/aas/full/2000/04/ds7983/ds7983.html}, journal = {Astron. Astrophys. Suppl. Ser.}, keywords = {recombination}, pages = {85--94}, posted-at = {2009-11-08 06:53:41}, priority = {2}, title = {Recombination coefficients for C II lines}, url = {http://aas.aanda.org/index.php?option=article&access=standard&Itemid=129&url=/articles/aas/full/2000/04/ds7983/ds7983.html}, volume = {142} }

TY - JOUR ID - citeulike:6083690 L3 - citeulike-article-id:6083690 N2 - Effective recombination coefficients are given for C II transitions between doublet states. The calculations are carried out in the temperature range $500 - 20\,000\;{K}$ and for an electron density of 10^4 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 $n \leq 15$ and total orbital angular momentum $L \leq 4$. The effect of moving the resonance features to their experimentally determined positions is also investigated and found to be important at low temperatures. JF - Astron. Astrophys. Suppl. Ser. EP - 94 TI - Recombination coefficients for C II lines VL - 142 SP - 85 KW - recombination AU - Davey, AR AU - Storey, PJ AU - Kisielius, R UR - http://aas.aanda.org/index.php?option=article&access=standard&Itemid=129&url=/articles/aas/full/2000/04/ds7983/ds7983.html ER -