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Titlebook: Clusters and Groups of Galaxies; International Meetin F. Mardirossian,G. Giuricin,M. Mezzetti Book 1984 D. Reidel Publishing Company, Dordr

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楼主: T-cell
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https://doi.org/10.1007/978-3-8351-9227-0 A concentration of galaxies, apparently coincident with 2151–5805 on the sky, is found to lie in the background at a higher redshift, illustrating how the knowledge of redshifts can resolve structure in three dimensions. Much faster and more objective automatic methods of determining the redshifts are currently being developed.
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The Spatial and Peculiar Velocity Distribution of Galaxies within 80 MPC,vertically through Figure 1. The other empty zone is caused by the gap in the catalogues between declinations −17°.5 to −2°.5. The 2-dimensional distribution in Figure 1 gives a strong visual impression of filamentary structure on angular scales up to a radian and more.
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Kurt Magnus,Karl Popp,Walter Sextronly composed of spirals. The possible connection of a cloud of galaxies surrounding the cluster A569, the new filament in Gemini and the Linx-Ursa Major supercluster with the Perseus supercluster is briefly discussed.
发表于 2025-3-31 09:15:33 | 显示全部楼层
A Redshift Survey in the Linx Gemini Region,nly composed of spirals. The possible connection of a cloud of galaxies surrounding the cluster A569, the new filament in Gemini and the Linx-Ursa Major supercluster with the Perseus supercluster is briefly discussed.
发表于 2025-3-31 15:17:17 | 显示全部楼层
Superclusters,dimensions ranging from tens of kiloparsecs to hundreds of Megaparsecs. The rich clusters may be the largest bound structures. The superclusters look largely unrelaxed: they have rarely a well-defined centre; their relatively small internal random motions indicate crossing times along the larger dia
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