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Radiation Charge Exchange and Radiation Ion-Atom Recombination as a Source of Continual E-M Radiation from Astrophysical Plasma

Published online by Cambridge University Press:  07 August 2017

A.A. Mihajlov
Affiliation:
Institute of Physics, P.O. Box 57, 11001 Beograd, Yugoslavia
M.S. Dimitrijevic
Affiliation:
Astronomical Observatory, Volgina 7, 11050 Beograd, Yugoslavia
A.M. Ermolaev
Affiliation:
Departement of Physics, University of Durham, Science Laboratories, Durham DH1 3LE, UK

Extract

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We show that for the study of emission from weakly ionized low temperature hydrogen plasmas, the processes A+ + AA+ + A + ħω and A+ + AA+2 + ħω (where A denotes a neutral atom in ground state and, A+ and A+2 atomic and molecular ions) must be treaded as a source of continual electro–magnetic radiation from low temperature plasma. Both reaction channels are treated separately and the corresponding total and separate spectral intensities are determined for hydrogen plasma at T < 10000K. The obtained results have been also compared with the corresponding spectral intensities for electron–ion bremsstrahlung and electron–ion photorecombination.

Type
III. Highlights on the Nebulae
Copyright
Copyright © Kluwer 1993 

References

Mihajlov, A.A., Dimitrijevic, M.S., and Ermolaev, A.M. (1992), in press.Google Scholar