| Display title | Astronomy:OVV quasar |
| Default sort key | OVV quasar |
| Page length (in bytes) | 1,739 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 574251 |
| 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>JOpenQuest |
| Date of page creation | 12:32, 6 February 2024 |
| Latest editor | imported>JOpenQuest |
| Date of latest edit | 12:32, 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. | An optically violent variable quasar (often abbreviated as OVV quasar) is a type of highly variable quasar. It is a subtype of blazar that consists of a few rare, bright radio galaxies, whose visible light output can change by 50% in a day. OVV quasars have essentially become unified with highly polarized... |
