| Display title | Astronomy:Low-ionization nuclear emission-line region |
| Default sort key | Low-ionization nuclear emission-line region |
| Page length (in bytes) | 12,096 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 717378 |
| 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>John Stpola |
| Date of page creation | 06:04, 6 February 2024 |
| Latest editor | imported>John Stpola |
| Date of latest edit | 06:04, 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. | A low-ionization nuclear emission-line region (LINER) is a type of galactic nucleus that is defined by its spectral line emission. The spectra typically include line emission from weakly ionized or neutral atoms, such as O, O+, N+, and S+. Conversely, the spectral line emission from strongly ionized... |
