Publication Date:
2013-09-04
Description:
Author(s): S. J. Jin, Y. B. Wang, J. Su, S. Q. Yan, Y. J. Li, B. Guo, Z. H. Li, S. Zeng, G. Lian, X. X. Bai, W. P. Liu, H. Yamaguchi, S. Kubono, J. Hu, D. Kahl, H. S. Jung, J. Y. Moon, C. S. Lee, T. Teranishi, H. W. Wang, H. Ishiyama, N. Iwasa, T. Komatsubara, and B. A. Brown Background: In presolar low-density graphite grains, an extraordinarily large 22 Ne/ 20 Ne ratio or even nearly pure 22 Ne is found, pointing to the condensation of radioactive 22 Na in grains. Supernovae and neon-rich novae are the main events that produce 22 Na via the explosive hydrogen burning process... [Phys. Rev. C 88, 035801] Published Tue Sep 03, 2013
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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