| Display title | Astronomy:BY Draconis variable |
| Default sort key | By Draconis Variable |
| Page length (in bytes) | 4,197 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 374064 |
| 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>Steve Marsio |
| Date of page creation | 09:16, 26 September 2021 |
| Latest editor | imported>Steve Marsio |
| Date of latest edit | 09:16, 26 September 2021 |
| 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. | BY Draconis variables are variable stars of late spectral types, usually K or M, and typically belong to the main sequence. The name comes from the archetype for this category of variable star system, BY Draconis. They exhibit variations in their luminosity due to rotation of the star coupled with starspots... |
