| Display title | Astronomy:Galaxy groups and clusters |
| Default sort key | Galaxy Groups And Clusters |
| Page length (in bytes) | 14,244 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 375172 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
| Number of redirects to this page | 0 |
| Counted as a content page | Yes |
| Page image |  |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>HamTop |
| Date of page creation | 14:17, 6 February 2024 |
| Latest editor | imported>HamTop |
| Date of latest edit | 14:17, 6 February 2024 |
| Total number of edits | 1 |
| Recent number of edits (within past 90 days) | 0 |
| Recent number of distinct authors | 0 |
Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | Galaxy groups and clusters are the largest known gravitationally bound objects to have arisen thus far in the process of cosmic structure formation. They form the densest part of the large-scale structure of the Universe. In models for the gravitational formation of structure with cold dark matter, the... |
