Tham khảo Quá_trình_p

  1. ↑ Burbidge, E. M.; Burbidge, G. R.; Fowler, W. A.; Hoyle, F. (1957). “Synthesis of the Elements in Stars”. Reviews of Modern Physics 29 (4): 547–650. Bibcode:1957RvMP...29..547B. doi:10.1103/RevModPhys.29.547. 
  2. ↑ Cameron, A. G. W. (1957). “Nuclear Reactions in Stars and Nucleogenesis”. Publications of the Astronomical Society of the Pacific 69 (408): 201–222. Bibcode:1957PASP...69..201C. JSTOR 40676435. doi:10.1086/127051. 
  3. ↑ Arnould, M.; Goriely, S. (2003). “The p-Process of Stellar Nucleosynthesis: Astrophysics and Nuclear Physics Status”. Physics Reports 384 (1–2): 1–84. Bibcode:2003PhR...384....1A. doi:10.1016/S0370-1573(03)00242-4. 
  4. ↑ Rauscher, T. (2010). “Origin of p-Nuclei in Explosive Nucleosynthesis”. Proceedings of Science. NIC XI (59). Bibcode:2010arXiv1012.2213R. arXiv:1012.2213.