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The Hubble Flow: Why Does the Cosmological Expansion Preserve Its Kinematical Identity from a Few Mpc Distance to the Observation Horizon?

✍ Scribed by I.D. Karachentsev; A.D. Chernin; P. Teerikorpi


Book ID
111572104
Publisher
Springer
Year
2003
Tongue
English
Weight
241 KB
Volume
46
Category
Article
ISSN
0571-7256

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