| Display title | Astronomy:Bipolar outflow |
| Default sort key | Bipolar outflow |
| Page length (in bytes) | 8,861 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 373895 |
| 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>Jport |
| Date of page creation | 04:45, 19 July 2022 |
| Latest editor | imported>Jport |
| Date of latest edit | 04:45, 19 July 2022 |
| 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. | A bipolar outflow comprises two continuous flows of gas from the poles of a star. Bipolar outflows may be associated with protostars (young, forming stars), or with evolved post-AGB stars (often in the form of bipolar nebulae). |
