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Karachentsev, I.D., Chernin, A.D. and Teerikorpi, P. (2003) The Hubble Flow: Why Does the Cosmological Expansion Preserve Its Kinematical Identity from a Few Mpc Distance to the Observation Horizon? Astrophysics, 46, 399-414.
https://doi.org/10.1023/B:ASYS.0000003255.06980.c0

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