Abstract
Physical processes that can, under cosmic conditions, give rise to emission whose spectrum peaks at some frequency are discussed in the context of the spectrum of the central extended component of a model brightness distribution for the radio galaxy 3C 234. This component is not detected at decameter wavelengths, probably due to the absorption of the radiation in the plasma in the source itself.
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Translated from Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) Zhurnal, Vol. 81, No. 5, 2004, pp. 411–417.
Original Russian Text Copyright © 2004 by Megn.
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Megn, A.V. Spectral characteristics of components of a model radio-brightness distribution for the radio galaxy 3C 234. Astron. Rep. 48, 374–379 (2004). https://doi.org/10.1134/1.1744937
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DOI: https://doi.org/10.1134/1.1744937