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?

2003-04-14

arxiv.org/abs/astro-ph/0304250v1

Astronomy and Astrophysics

Astrophysics

20 pages, 7 figures, submitted to Astrofizika

Scientific paper

The problem of the physical nature of the Hubble flow in the Local Volume ($D
< 10$ Mpc) stated by Sandage(1986, 1999) 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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