| Display title | Physics:Shock waves in astrophysics |
| Default sort key | Shock waves in astrophysics |
| Page length (in bytes) | 4,613 |
| Namespace ID | 3020 |
| Namespace | Physics |
| Page ID | 637679 |
| 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>AIposter |
| Date of page creation | 05:53, 5 February 2024 |
| Latest editor | imported>AIposter |
| Date of latest edit | 05:53, 5 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. | Shock waves are common in astrophysical environments.
Because of the low ambient density, most astronomical shocks are collisionless. This means that the shocks are not formed by two-body Coulomb collisions, since the mean free path for these collisions is too large, often exceeding the size of the system... |
