Display title | Astronomy:PSR J0348+0432 |
Default sort key | PSR J0348+0432 |
Page length (in bytes) | 12,690 |
Namespace ID | 3024 |
Namespace | Astronomy |
Page ID | 468006 |
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>Wikisleeper |
Date of page creation | 08:44, 6 February 2024 |
Latest editor | imported>Wikisleeper |
Date of latest edit | 08:44, 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. | PSR J0348+0432 is a pulsar–white dwarf binary system in the constellation Taurus. It was discovered in 2007 with the National Radio Astronomy Observatory's Robert C. Byrd Green Bank Telescope in a drift-scan survey.
In 2013, a mass measurement for this neutron star was announced: slightly over two times... |