Radio Source Spectra and the Cosmological Red-shift

Mathematics – Logic

Scientific paper

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Scientific paper

RECENT spectral surveys of discrete radio sources have not revealed any significant dependence of spectral index on apparent intensity1-3. It is therefore of interest to determine the way in which the mean observed spectral index depends on flux density, when the effects of cosmological red-shift are taken into account. We shall choose, by way of example, a hyperbolic world model.

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