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Uspekhi Fizicheskikh Nauk, 2014, Volume 184, Number 7, Pages 767–774
DOI: https://doi.org/10.3367/UFNr.0184.201407f.0767 (Mi ufn4820) 		 
This article is cited in 2 scientific papers (total in 2 papers)

METHODOLOGICAL NOTES

The Hubble flow: an observer's perspective

A. V. Toporensky, S. B. Popov

Sternberg Astronomical Institute, Lomonosov Moscow State University
Full-text PDF (665 kB) Citations (2)
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DOI: https://doi.org/10.3367/UFNr.0184.201407f.0767
Abstract: This paper discusses some aspects of cosmological expansion as viewed by an observer. It identifies the rate of change of the angular distance $v_\Theta$ with respect to the observer's clock as a crucial quantity in properly understanding the expansion. Using this quantity and the angular distance, in addition to the traditional approach to visualization, provides a more vivid picture of the cosmological expansion and is key for adequately visualizing it.
Received: September 2, 2013
Revised: October 15, 2013
Accepted: October 15, 2013
English version:
Physics–Uspekhi, 2014, Volume 57, Issue 7, Pages 708–713
DOI: https://doi.org/10.3367/UFNe.0184.201407f.0767
Bibliographic databases:
Document Type: Article
PACS: 98.62.Py, 98.80.-k, 98.80.Es
Language: Russian
Citation: A. V. Toporensky, S. B. Popov, “The Hubble flow: an observer's perspective”, UFN, 184:7 (2014), 767–774; Phys. Usp., 57:7 (2014), 708–713
Citation in format AMSBIB
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    • This publication is cited in the following 2 articles:
    Citing articles in Google Scholar: Russian citations, English citations
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