Tham khảo Chu trình CNO

  1. 1 2 Salaris, Maurizio; Cassisi, Santi (2005). Evolution of Stars and Stellar Populations. John Wiley and Sons. tr. 119–121. ISBN 0-470-09220-3. 
  2. ↑ Reid, I. Neill; Hawley, Suzanne L. (2005). “The Structure, Formation and Evolution of Low-Mass Stars and Brown Dwarfs – Energy Generation”. New Light on Dark Stars: Red Dwarfs, Low-Mass Stars, Brown Dwarfs. Springer-Praxis Books in Astrophysics and Astronomy (ấn bản 2). Springer Science & Business Media. tr. 108–111. ISBN 3-540-25124-3. 
  3. ↑ Schuler, S. C.; King, J. R.; The, L.-S. (2009). “Stellar Nucleosynthesis in the Hyades Open Cluster”. The Astrophysical Journal 701 (1): 837–849. Bibcode:2009ApJ...701..837S. arXiv:0906.4812. doi:10.1088/0004-637X/701/1/837. 
  4. 1 2 von Weizsäcker, Carl F. (1937). “Über Elementumwandlungen in Innern der Sterne I” [On Transformations of Elements in the Interiors of Stars I]. Physikalische Zeitschrift 38: 176–191. 
  5. 1 2 von Weizsäcker, Carl F. (1938). “Über Elementumwandlungen in Innern der Sterne II” [On Transformations of Elements in the Interiors of Stars II]. Physikalische Zeitschrift 39: 633–646. 
  6. 1 2 3 Bethe, Hans A. (1939). “Energy Production in Stars”. Physical Review 55 (1): 103. doi:10.1103/PhysRev.55.103. 
  7. 1 2 3 Bethe, Hans A. (1939). “Energy Production in Stars”. Physical Review 55 (5): 434–456. doi:10.1103/PhysRev.55.434. 
  8. ↑ Bethe, Hans A.; Bacher, Robert (1936). “Nuclear Physics, A: Stationary States of Nuclei” (PDF). Reviews of Modern Physics 8 (2): 82–229. doi:10.1103/RevModPhys.8.82. 
  9. ↑ Bethe, Hans A. (1937). “Nuclear Physics, B: Nuclear Dynamics, Theoretical”. Reviews of Modern Physics 9 (2): 69–244. doi:10.1103/RevModPhys.9.69. 
  10. ↑ Bethe, Hans A.; Livingston, Milton S. (1937). “Nuclear Physics, C: Nuclear Dynamics, Experimental”. Reviews of Modern Physics 9 (2): 245–390. doi:10.1103/RevModPhys.9.245. 
  11. ↑ Bardi, Jason Socrates (23 tháng 1 năm 2008). “Landmarks: What Makes the Stars Shine?”. Physical Review Focus 21 (3). Truy cập ngày 26 tháng 11 năm 2018. 
  12. 1 2 3 Krane, Kenneth S. (1988). Introductory Nuclear Physics. John Wiley & Sons. tr. 537. ISBN 0-471-80553-X. 
  13. 1 2 Ray, Alak (2010). “Massive Stars as Thermonuclear Reactors and their Explosions Following Core Collapse”. Trong Goswami, Aruna; Reddy, B. Eswar. Principles and Perspectives in Cosmochemistry. Springer Science & Business Media. tr. 233. ISBN 9783642103681. 
  14. ↑ Wapstra, Aaldert; Audi, Georges (18 tháng 11 năm 2003). “The 2003 Atomic Mass Evaluation”. Atomic Mass Data Center. Truy cập ngày 25 tháng 10 năm 2011. 
  15. ↑ LUNA Collaboration; Lemut, A.; Bemmerer, D.; Confortola, F.; Bonetti, R.; Broggini, C.; Corvisiero, P.; Costantini, H.; Cruz, J.; Formicola, A.; Fülöp, Zs.; Gervino, G. và đồng nghiệp (2006). “First measurement of the 14N(p,γ)15O cross section down to 70 keV”. Physics Letters B 634: 483–487. Bibcode:2006PhLB..634..483L. arXiv:nucl-ex/0602012. doi:10.1016/j.physletb.2006.02.021. 
  16. ↑ Scheffler, Helmut; Elsässer, Hans (1990). Die Physik der Sterne und der Sonne [The Physics of the Stars and the Sun]. Bibliographisches Institut (Mannheim, Wien, Zürich). ISBN 3-411-14172-7.