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Phys. Rev. C 73, 049907(E) (2006) [2 pages]Erratum: Astrophysically important 26Si states studied with the (3He, n) reaction and the 25Al(p,
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)26Si reaction rates in explosive hydrogen burning environments [Phys. Rev. C 70, 065805 (2004)]| URL: | http://link.aps.org/doi/10.1103/PhysRevC.73.049907 | |
| DOI: | 10.1103/PhysRevC.73.049907 | |
| PACS: |
12.38.Aw;
13.60.Le;
14.20.Gk;
99.10.Cd
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| KEYWORDS: | nuclei with mass number 20 to 38, stellar internal processes, nucleosynthesis, nuclear energy levels, helium 3-nucleus reactions, proton radiative capture | |
See Also
Astrophysically important 26Si states studied with the (3He,n) reaction and the 25Al(p,
)26Si reaction rates in explosive hydrogen burning environments
Y. Parpottas, S. M. Grimes, S. Al-Quraishi et al.
Phys. Rev. C 70, 065805 (2004)
REFERENCES (3)
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C. Iliadis, L. Buchmann, P. M. Endt, H. Herndl, and M. Wiescher, Phys. Rev. C 53, 475 (1996).
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C. Iliadis, J. M. D'Auria, S. Starrfield, W. J. Thompson, and M. Wiescher, Astrophys. J., Suppl. Ser. 134, 151 (2001).
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J. A. Caggiano et al., Phys. Rev. C 65, 055801 (2002).
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- Astrophysically important 26Si states studied with the (3He,n) reaction and the 25Al(p,)26Si reaction rates in explosive hydrogen burning environments
Y. Parpottas, S. M. Grimes, S. Al-Quraishi et al.
Phys. Rev. C 70, 065805 (2004)
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