Publication Date:
2016-05-24
Description:
Author(s): Q. Li, J. Görres, R. J. deBoer, G. Imbriani, A. Best, A. Kontos, P. J. LeBlanc, E. Uberseder, and M. Wiescher Background: The CNO cycle is the main energy source in stars more massive than our sun; it defines the energy production and the cycle time that lead to the lifetime of massive stars, and it is an important tool for the determination of the age of globular clusters. In our sun about 1.6% of the tota… [Phys. Rev. C 93, 055806] Published Mon May 23, 2016
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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