Experimentally Well-Constrained Masses of 27P and 27S: Implications for Studies of Explosive Binary Systems
L. J. Sun,X. X. Xu,S. Q. Hou,C. J. Lin,J. Jose,J. Lee,J. J. He,Z. H. Li,J. S. Wang,C. X. Yuan,F. Herwig,J. Keegans,T. Budner,D. X. Wang,H. Y. Wu,P. F. Liang,Y. Y. Yang,Y. H. Lam,P. Ma,F. F. Duan,Z. H. Gao,Q. Hu,Z. Bai,J. B. Ma,J. G. Wang,F. P. Zhong,C. G. Wu,D. W. Luo,Y. Jiang,Y. Liu,D. S. Hou,R. Li,N. R. Ma,W. H. Ma,G. Z. Shi,G. M. Yu,D. Patel,S. Y. Jin,Y. F. Wang,Y. C. Yu, Q. W. Zhou,P. Wang,L. Y. Hu,X. Wang,H. L. Zang,P. J. Li,Q. Q. Zhao,H. M. Jia,L. Yang,P. W. Wen,F. Yang,M. Pan,X. Y. Wang,Z. G. Hu,R. F. Chen,M. L. Liu,W. Q. Yang,Y. M. Zhao Physics Letters B（2018）
Key words
Masses of P-27 and S-27,Si-26(p, gamma)P-27 reaction,X-ray bursts,Nova outbursts
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