The Hubble Flow: Why Does the Cosmological Expansion Preserve Its Kinematical Identity from a Few Mpc Distance to the Observation Horizon?
Author： Karachentsev I. D.
Publisher： Springer Publishing Company
ISSN： 0571-7256
Source： Astrophysics, Vol.46, Iss.4, 2003-10, pp. : 399-414
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
Related content
Access to resources
Recommend
