Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.291..113r&link_type=abstract
Astrophysics and Space Science, v. 291, Issue 2, p. 113-122 (2004).
Astronomy and Astrophysics
Astrophysics
5
Radio Recombination Lines, Cii Regions, Dielectronic-Like Recombination, Populations
Scientific paper
The intensities of carbon radio recombination lines (RRL’s) are definedallowing for the effect of dielectronic-like recombination. The rate ofdielectronic-like recombination is calculated as functions of line number,electron density and temperature accurate to 0.05. Following from the balanceequation solutions for populations, the RRL intensities are analytically foundby the method of successive approximations to an accuracy of 0.15. Theobservations of carbon RRL’s are analyzed toward Cassiopeia A. The averageelectron temperature, density, expanded CII region lengths and inaccuraciesare found with the experimental values of RRL widths and intensities.
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