| Display title | Astronomy:High-velocity cloud |
| Default sort key | High-velocity cloud |
| Page length (in bytes) | 27,280 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 591666 |
| 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>Steve2012 |
| Date of page creation | 03:47, 27 June 2023 |
| Latest editor | imported>Steve2012 |
| Date of latest edit | 03:47, 27 June 2023 |
| 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. | High-velocity clouds (HVCs) are large collections of gas found throughout the galactic halo of the Milky Way. Their bulk motions in the local standard of rest have velocities which are measured in excess of 70–90 km s−1. These clouds of gas can be massive in size, some on the order of millions of... |
