The Radio Recombination Line Intensities Of Atoms And Ions: Helium, Carbon And Oxygen

Details The Radio Recombination Line Intensities Of Atoms And Ions: Helium, Carbon And Oxygen The Radio Recombination Line Intensities Of Atoms And Ions: Helium, Carbon And Oxygen

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.300..357r&link_type=abstract

Astrophysics and Space Science, Volume 300, Issue 4, pp.357-366

Astronomy and Astrophysics

Astrophysics

Radio Recombination Lines, Dielectronic Recombination

Scientific paper

The radio recombination line intensities of heavy elements of helium, carbon and oxygen are calculated with accounting for dielectronic recombination. Dielectronic recombination rates are determined accurate to the second order of a perturbation theory and the rates are described as function of principal quantum number for helium-like atom or ion. Balance equations are solved for the departure coefficients from LTE bn. The collision and spontaneous transition rates are accounted for the balance equations, in which non-equilibrium distribution source is dielectronic recombination. Non-equilibrium amplification coefficients are found as functions of a medium temperature, density and ion charge z = 1 3 for radio recombination lines.

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