Dielectronic recombination at low temperatures. IV - Recombination coefficients for neon

Details Dielectronic recombination at low temperatures. IV - Recombination coefficients for neon Dielectronic recombination at low temperatures. IV - Recombination coefficients for neon

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...69..123n&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 69, no. 1, April 1987, p. 123-133.

Astronomy and Astrophysics

Astrophysics

67

Electron Energy, Electron Recombination, Gas Ionization, Nebulae, Neon, Recombination Coefficient, Low Temperature, Transition Probabilities

Scientific paper

Effective dielectronic recombination coefficients are calculated for the total recombination, as well as for selected lines and ground and metastable terms of several ionization stages of neon. The effective recombination coefficients are fitted to a convenient function of temperature in the range 103 to 6×104K. The lack of experimental data for energy levels introduces considerable uncertainties in the calculated recombination rates.

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