The β-delayed α-spectrum of 16N, and its role in defining the astrophysical cross section for 12C(α,γ)16O-Reference-Cited by-同舟云学术

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The β-delayed α-spectrum of 16N, and its role in defining the astrophysical cross section for 12C(α,γ)16O

Published:1995-05 Issue:1 Volume:588 Page:c295-c304
ISSN:0375-9474
Container-title:Nuclear Physics A
language:en
Short-container-title:Nuclear Physics A

Author:

Barnes C.A.

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics

Reference29 articles.

1. Essays in Nuclear Astrophysics;Barnes,1982

2. Nucleosynthesis in massive stars and the 12C(α, γ)16O reaction rate

3. S.E. Woosley and T.A. Weaver, in the proceedings of the conference, Nuclei in the Cosmos III, M. Busso, R. Gallino, C.M. Raiteri, American Institute of Physics, to be published.

Cited by 4 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Frontiers in nuclear astrophysics;Progress in Particle and Nuclear Physics;2016-07

2. 16O Coulomb dissociation: towards a new means to determine the 12C+α fusion rate in stars;Physics Letters B;2005-06

3. The evolution and explosion of massive stars;Reviews of Modern Physics;2002-11-07

4. The formation of high-mass black holes in low-mass X-ray binaries;New Astronomy;1999-07

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