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Dielectronic Recombination in the Gaseous Nebulae as a Cooling Process
Published online by Cambridge University Press: 07 August 2017
Extract
The dielectronic recombination (DR) is of importance at ‘low’ (nebular) temperature. This process leads to cooling the electron gas in nebulae. The cooling rate by recombination of ion X+n is
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- III. Highlights on the Nebulae
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