| Display title | Astronomy:Neutron star spin-up |
| Default sort key | Neutron star spin-up |
| Page length (in bytes) | 1,934 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 376138 |
| 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>Steve Marsio |
| Date of page creation | 10:55, 6 February 2024 |
| Latest editor | imported>Steve Marsio |
| Date of latest edit | 10:55, 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. | Neutron star spin up is the name given to the increase in rotational speed over time first noted in Cen X-3 and Her X-1 but now observed in other X-ray pulsars. In the case of Cen X-3, the pulse period is decreasing over a timescale of 3400 years (defined as $ P/{\dot {P}} $, where $ P $ is the... |
