Abstract
A new mechanism is proposed for non-thermal radio emission, which depends upon the scattering of photons within an unstable counter-streaming plasma. This mechanism may play a dominant role in several phenomena:(i)the short-wave emission from quasi-stellar sources;(ii)the emission from symmetric supernova nebulae in the early stages of the nebular expansion;(iii)maintenance or modification of the 3 °K black-body background radiation of the Universe.
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