| Display title | Astronomy:Cygnus X-3 |
| Default sort key | Cygnus X-3 |
| Page length (in bytes) | 14,161 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 444508 |
| 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>AIposter |
| Date of page creation | 10:31, 6 February 2024 |
| Latest editor | imported>AIposter |
| Date of latest edit | 10:31, 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. | Cygnus X-3 is a high-mass X-ray binary (HMXB), one of the stronger binary X-ray sources in the sky. It is often considered to be a microquasar, and it is believed to be a compact object in a binary system which is pulling in a stream of gas from an ordinary star companion. It is one of only two known... |
