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Tidal compression of the Local Supercluster
The effects of the extended low density region behind the Local Supercluster on various approaches to determining the motion of the Local Group are discussed. In particular it is shown that the method of comparing the local and global values of the Hubble constant could overestimate the infall veloc...
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Published in: | Monthly notices of the Royal Astronomical Society 1983-01, Vol.202 (1), p.7P-10P |
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container_title | Monthly notices of the Royal Astronomical Society |
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creator | Ftaclas, Christ |
description | The effects of the extended low density region behind the Local Supercluster on various approaches to determining the motion of the Local Group are discussed. In particular it is shown that the method of comparing the local and global values of the Hubble constant could overestimate the infall velocity of the Local Group by 100 km s−1. These considerations are applied to the infall velocity determined from the Fornax and Grus clusters by Aaronson et al. |
doi_str_mv | 10.1093/mnras/202.1.7P |
format | article |
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ispartof | Monthly notices of the Royal Astronomical Society, 1983-01, Vol.202 (1), p.7P-10P |
issn | 0035-8711 1365-2966 |
language | eng |
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source | EZB Electronic Journals Library; Oxford Open Access Journals |
title | Tidal compression of the Local Supercluster |
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