| Display title | Astronomy:IRAS 18162−2048 |
| Default sort key | IRAS 18162-2048 |
| Page length (in bytes) | 2,935 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 717123 |
| 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>WikiGary |
| Date of page creation | 03:52, 27 June 2023 |
| Latest editor | imported>WikiGary |
| Date of latest edit | 03:52, 27 June 2023 |
| 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. | IRAS 18162-2048 is a far-infrared source discovered by IRAS spacecraft in 1983. It is associated with a massive (~10 solar masses) protostar, which accretes gas from a disk that surrounds it. IRAS 18162-2048 emits two collimated radio jets along its axis of rotation. The jets are made of chains of radio... |
