| | Galaxies and the Universe - Large-Scale Structure |
 | | Redshift surveys are now available for Abell clusters (since velocity dispersions require multiple objects anyway), for Zwicky galaxies and their southern counterparts from the CfA and SSRS groups; and for selected deep "postage-stamp" areas. |
 | | Hamilton, Kluwer 1998), a cluster or other structure embedded in the Hubble expansion will have distinct signatures in a space-redshift slice depending on whether it is overall expanding (even if decelerating from the general expansion), just turning around from the expansion, or collapsing toward a relaxed structure. |
 | | As the cluster finally decouples from the Hubble flow, collapses, and eventually becomes dynamically relaxed, we get the familiar "finger-of-God" effect in which the internal velocities become very large, much larger than the differential Hubble flow across the cluster since the depth of the potential well is significant. |
| www.astr.ua.edu /keel/galaxies/largescale.html (1770 words) |