| Display title | Astronomy:Canis Major Overdensity |
| Default sort key | Canis Major Overdensity |
| Page length (in bytes) | 9,685 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 718985 |
| 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 |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>Smart bot editor |
| Date of page creation | 06:27, 6 February 2024 |
| Latest editor | imported>Smart bot editor |
| Date of latest edit | 06:27, 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. | The Canis Major Overdensity (CMa Overdensity) or Canis Major Dwarf Galaxy (CMa Dwarf) is a disputed dwarf irregular galaxy in the Local Group, located in the same part of the sky as the constellation Canis Major.
The supposed small galaxy contains a relatively high percentage of red giants and is thought... |
