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The form of logN-logS relation in the domain of strong flux densities

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Abstract

The slope formed in the curves of counts in a strong flux density region can be explained by a constraint on the flux density of radio sources and the spread of their spectral indices.

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References

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  1. Sternberg State Astronomical Institute, Moscow, USSR

    V. R. Amirkhanyan

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  1. V. R. Amirkhanyan
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Amirkhanyan, V.R. The form of logN-logS relation in the domain of strong flux densities. Astrophys Space Sci 108, 319–322 (1985). https://doi.org/10.1007/BF01068258

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  • DOI: https://doi.org/10.1007/BF01068258

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