Nature of Sources of Cosmic Synchrotron Radiation

Physics

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Scientific paper

FROM an analysis of the emission bands in the spectra of 3C273 and 3C48 described in refs. 1 and 2, it may be concluded that the size of the gas envelopes around `radio stars' (emitting continuous spectrum) must be at least 1020 cm. Indeed, the total energy radiated in any emission band is L α N2er3x½, where Neis the electron density, r is the radius of the gas envelope and x is the non-uniformity factor which has been assumed to be ~ 10-2.

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