2020
DOI: 10.48550/arxiv.2004.01427
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Anton N. Baushev

Abstract: The gravitational field of a massive object (for instance, of a galaxy group or cluster) disturbs the Hubble stream, decreasing its speed. Dependence v(r 0 ) of the radial velocity of the stream from the present-day radius r 0 can be directly observed and may provide valuable information about the cluster properties. We offer an exact analytical relationship v(r 0 ) for a spherically-symmetric system.

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