The Hubble Flow Why Does the Cosmological Expansion Preserve its Kinematical Identity from a Few MPC Distance to the Observation Horizon?

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dc.creatorKarachentsev, Igor D.
dc.creatorChernin, Arthur D.
dc.creatorTeerikorpi, Pekka
dc.date2003-04-14
dc.date.accessioned2026-07-25T18:58:08Z
dc.descriptionThe 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.
dc.description20 pages, 7 figures, submitted to Astrofizika
dc.identifierhttps://arxiv.org/abs/astro-ph/0304250
dc.identifierhttp://arxiv.org/abs/astro-ph/0304250
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/60202
dc.subjectAstrophysics
dc.titleThe Hubble Flow Why Does the Cosmological Expansion Preserve its Kinematical Identity from a Few MPC Distance to the Observation Horizon?
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