Display title | Astronomy:Galactic corona |
Default sort key | Galactic Corona |
Page length (in bytes) | 4,650 |
Namespace ID | 3024 |
Namespace | Astronomy |
Page ID | 411000 |
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>Gametune |
Date of page creation | 13:35, 17 May 2022 |
Latest editor | imported>Gametune |
Date of latest edit | 13:35, 17 May 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. | The terms galactic corona and gaseous corona have been used in the first decade of the 21st century to describe a hot, ionised, gaseous component in the galactic halo of the Milky Way. A similar body of very hot and tenuous gas in the halo of any spiral galaxy may also be described by these terms... |