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Cosmic rotation and the inertial system

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Abstract

A second order aberration term is employed for a determination of cosmic rotation from extremely precise relative positions of pairs of quasars. The value derived (ω o/Ho<10−5) corresponds with values derived from fluctuations of cosmic background radiation.

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Authors and Affiliations

  1. Zentralinstitut für Astrophysik, Rosa-Luxemburg-Str. 17a, 1591, Potsdam, DDR

    G. Ruben

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  1. G. Ruben
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Ruben, G. Cosmic rotation and the inertial system. Astrophys Space Sci 177, 465–470 (1991). https://doi.org/10.1007/BF00643720

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  • DOI: https://doi.org/10.1007/BF00643720

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