| Display title | Astronomy:IRAS 19475+3119 |
| Default sort key | IRAS 19475+3119 |
| Page length (in bytes) | 7,715 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 499883 |
| 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>AIposter |
| Date of page creation | 14:39, 2 August 2025 |
| Latest editor | imported>AIposter |
| Date of latest edit | 14:39, 2 August 2025 |
| 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 19475+3119 is a protoplanetary nebula in the constellation of Cygnus, 15,000 light-years away. The central star, V2513 Cygni, is an F-type post-AGB star.
The brightest portion of the nebula shows a quadrupolar structure, with elongated bipolar lobes, all surrounded by a faint halo.
The distance... |