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  1. ↑ Girardi, L.; Bressan, A.; Bertelli, G.; Chiosi, C. (2000). "Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 Msun, and from Z=0.0004 to 0.03". Astronomy and Astrophysics Supplement. 141: 371–383. doi:10.1051/aas:2000126.CS1 maint: multiple names: authors list (link)
  2. 1 2 Clayton, Donald. Principles of Stellar Evolution and Nucleosynthesis, (1983)
  3. ↑ Siess L. (2007). "Evolution of massive AGB stars. I. Carbon burning phase". Astronomy and Astrophysics. 476: 893–909. doi:10.1051/0004-6361:20053043.
  4. ↑ Hernandez, G.; และคณะ (December 2006). "Rubidium-Rich Asymptotic Giant Branch Stars". Science. 314 (5806): 1751–1754. arXiv:arXiv:astro-ph/0611319 Check |arxiv= value (help). doi:10.1126/science.1133706. PMID 17095658. Explicit use of et al. in: |author= (help)

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