degenerate star
A star that has collapsed to a high density so that *degeneracy pressure is its main support against further collapse. Collapse to a degenerate state occurs either after nuclear fuel is exhausted, as in white dwarfs and neutron stars, or, as in brown dwarfs, which have insufficient mass to raise the core temperature high enough to ignite hydrogen.... ...
Access to the complete content on Oxford Reference requires a subscription or purchase. Public users are able to search the site and view the abstracts and keywords for each book and chapter without a subscription.
Please subscribe or login to access full text content.
If you have purchased a print title that contains an access token, please see the token for information about how to register your code.
For questions on access or troubleshooting, please check our FAQs, and if you can''t find the answer there, please contact us.