Electron temperature dependence of the recombination coefficient in neon

1965 ◽  
Vol 53 (6) ◽  
pp. 657-658 ◽  
Author(s):  
R.L. Taylor ◽  
S.B. Herskovitz ◽  
N. Farhat
1961 ◽  
Vol 121 (5) ◽  
pp. 1391-1400 ◽  
Author(s):  
C. L. Chen ◽  
C. C. Leiby ◽  
L. Goldstein

2000 ◽  
Vol 27 (4) ◽  
pp. 481-484 ◽  
Author(s):  
Robert Peverall ◽  
Stefan Rosén ◽  
Mats Larsson ◽  
James R. Peterson ◽  
Rolf Bobbenkamp ◽  
...  

1983 ◽  
Vol 103 ◽  
pp. 513-514
Author(s):  
H. Nussbaumer ◽  
P.J. Storey

Dielectronic recombination coefficients have been calculated for some ions of C, N and O by Storey (1981, Mon. Not. R. astr. Soc., 195, 27P). Using the same approach, we have extended those calculations to all other ions of C, N and O for which a dielectronic contribution to the total recombination coefficient might be expected at nebular temperatures. Recombination coefficients have been calculated in the temperature range from 5000 K up to the temperature at which the Burgess general formula becomes valid. The total dielectronic recombination coefficients are fitted to a simple function of the electron temperature.


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