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Angular size-redshift: Experiment and calculation

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Abstract

In this paper the next attempt is made to clarify the nature of the Euclidean behavior of the boundary in the angular size-redshift cosmological test. It is shown experimentally that this can be explained by the selection determined by anisotropic morphology and anisotropic radiation of extended radio sources. A catalogue of extended radio sources with minimal flux densities of about 0.01 Jy at 1.4 GHz was compiled for conducting the test. Without the assumption of their size evolution, the agreement between the experiment and calculation was obtained both in the ΛCDM model (Ω m = 0.27, Ω v = 0.73) and the Friedman model (Ω = 0.1).

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Authors and Affiliations

  1. Sternberg Astronomical Institute, Lomonosov Moscow State University, Moscow, 119992, Russia

    V. R. Amirkhanyan

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  1. V. R. Amirkhanyan
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Correspondence to V. R. Amirkhanyan.

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Original Russian Text © V.R. Amirkhanyan, 2014, published in Astrofizicheskii Byulleten, 2014, Vol. 69, No. 4, pp. 406–412.

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Amirkhanyan, V.R. Angular size-redshift: Experiment and calculation. Astrophys. Bull. 69, 383–389 (2014). https://doi.org/10.1134/S1990341314040026

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  • DOI: https://doi.org/10.1134/S1990341314040026

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