Level structure of 21Mg and the 20Na(p, γ)21Mg stellar reaction rate-Reference-Cited by-同舟云学术

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Level structure of 21Mg and the 20Na(p, γ)21Mg stellar reaction rate

Published:1992-02 Issue:1-2 Volume:537 Page:153-166
ISSN:0375-9474
Container-title:Nuclear Physics A
language:en
Short-container-title:Nuclear Physics A

Author:

Kubono S.,Funatsu Y.,Ikeda N.,Yasue M.,Nomura T.,Fuchi Y.,Kawashima H.,Kato S.,Miyatake H.,Orihara H.,Kajino T.

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics

Reference23 articles.

1. Explosive hydrogen burning

2. Proc. First Texas Symp. on relativistic astrophysics: Quasi-stellar sources and gravitational collapse;Hoyle,1965

3. A new estimate of the Ne-19(p, gamma) Na-20 and O-15(alpha, gamma) Ne-19 reaction rates at stellar energies

4. Experimental determination of the Ne-19(p, gamma)Na-20 reaction rate and the breakout problem from the hot CNO cycle

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3. Isospin symmetry in B(E2) values: Coulomb excitation study of Mg21;Physical Review C;2019-05-06

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