Աստղաֆիզիկա =Астрофизика =Astrophysics

The Hubble flow: why does the cosmological expansion preserve its kinematical identity from a few Mpc distance to the observation horizon?

Karachentsev, I. D. and 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? Աստղաֆիզիկա, 46 (4). pp. 491-508. ISSN 0571-1712

[img]
Preview
PDF
Download (3075Kb) | Preview
    Item Type: Article
    Additional Information: Хаббловский поток: почему космологическое расширение сохраняет свою кинематическую идентичность от расстояния в несколько Мпк до наблюдательного горизонта?
    Uncontrolled Keywords: Караченцев И. Д., Чернин А. Д., Терикорпи П., cosmology, expansion-galaxies, motions
    Subjects: Q Science > QB Astrophysics > Cosmogony. Cosmology
    Divisions: UNSPECIFIED
    Depositing User: SCIINFO FSL
    Date Deposited: 19 Jun 2013 08:32
    Last Modified: 25 Jun 2020 20:52
    URI: http://astro.asj-oa.am/id/eprint/676

    Actions (login required)

    View Item