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

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

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap.....46..399k&link_type=abstract

Astrophysics (English translation of Astrofizika), v. 46, Issue 4, p. 399-414 (2003).

Astronomy and Astrophysics

Astrophysics

4

Cosmology Expansion - Galaxies Motions

Scientific paper

The problem of the physical nature of the Hubble flow in the Local
Volume (D < 10 Mpc) stated by Sandage is studied. New observational
data on galaxy motions and matter distribution around the Local Group
and nearby similar systems are described. Dynamical models are discussed
on the basis of the recent data on cosmic vacuum or dark energy.

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