Tham khảo Quá_trình_đốt_cháy_carbon

  1. 1 2 Ryan, Sean G.; Norton, Andrew J. (2010). Stellar Evolution and Nucleosynthesis. Cambridge University Press. tr. 135. ISBN 978-0-521-13320-3.
  2. ↑ Clayton, Donald (1983). Principles of Stellar Evolution and Nucleosynthesis. University of Chicago Press. ISBN 978-0-226-10953-4.
  3. 1 2 Siess L. (2007). “Evolution of massive AGB stars. I. Carbon burning phase”. Astronomy and Astrophysics. 476 (2): 893–909. Bibcode:2006A&A...448..717S. doi:10.1051/0004-6361:20053043.
  4. ↑ Hernandez, G. (tháng 12 năm 2006). “Rubidium-Rich Asymptotic Giant Branch Stars”. Science. 314 (5806): 1751–1754. arXiv:astro-ph/0611319. Bibcode:2006Sci...314.1751G. doi:10.1126/science.1133706. PMID 17095658. Đã bỏ qua tham số không rõ |displayauthors= (gợi ý |display-authors=) (trợ giúp)
  5. 1 2 Rose,, William K. (1998). Advanced Stellar Astrophysics. Cambridge University Press. tr. 227–229. ISBN 978-0-521-58833-1.Quản lý CS1: dấu chấm câu dư (liên kết)
  6. 1 2 3 4 5 Camiel, W. H.; de Loore; C. Doom (1992). Camiel W. H. de Loore (biên tập). Structure and evolution of single and binary stars. Astrophysics and Space Science Library. Springer. tr. 95–97. ISBN 978-0-7923-1768-5.
  7. ↑ Rose (1998), pp. 229–234
  8. ↑ Camiel (1992), pp.97–98

Tài liệu tham khảo

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