ISSN:
1476-4687
Source:
Nature Archives 1869 - 2009
Topics:
Biology
,
Chemistry and Pharmacology
,
Medicine
,
Natural Sciences in General
,
Physics
Notes:
[Auszug] According to stellar evolution theory4,5, a sufficiently massive pre-supernova star is thought to develop a degenerate carbon-oxygen core of mass 1.4M, radius Rc 〉 108 cm, ??matter density pc 〈 2 1010 g cm?3 which becomes unstable to inverse p decay, and implodes to become a neutron star. The ...
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1038/261673a0
Permalink