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Rubin–Ford effect


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An apparent anisotropy in the expansion of the Universe on a scale of around 100 million l.y., as revealed by a study of the motions of a sample of spiral galaxies by the American astronomers Vera Cooper Rubin (1928– ) and William Kent Ford, Jr (1931– ). The reason that there is not a purely isotropic Hubble flow is because the Universe is not homogeneous on these scales.


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