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Electron Radiative Recombination

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Radiative recombination

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Electron radiative recombination is a chemical process whereby an electron reacts with a positive atomic ion to produce a neutral atom with the emission of a photon (i.e., radiation). Examples include electron reaction with H+ to produce a neutral H atom plus a photon; photons produced in this process are responsible for the red color of many low-density nebulae.

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Correspondence to Steven B. Charnley .

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© 2014 Springer-Verlag Berlin Heidelberg

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Charnley, S.B. (2014). Electron Radiative Recombination. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_498-3

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  • DOI: https://doi.org/10.1007/978-3-642-27833-4_498-3

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Online ISBN: 978-3-642-27833-4

  • eBook Packages: Springer Reference Physics and AstronomyReference Module Physical and Materials ScienceReference Module Chemistry, Materials and Physics

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