Ядерное горение углерода (Russian Wikipedia)

Analysis of information sources in references of the Wikipedia article "Ядерное горение углерода" in Russian language version.

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Girardi, L.; Bressan, A.; Bertelli, G.; Chiosi, C. Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 M_sun, and from Z=0.0004 to 0.03 (англ.) // Astronomy and Astrophysics : journal. — 2000. — Vol. 141. — P. 371—383. — doi:10.1051/aas:2000126.

http://abyss.uoregon.edu/~js/ast122/lectures/lec18.html Архивная копия от 14 февраля 2020 на Wayback Machine "Stars greater than 25 solar masses undergo a more violent end to their lives. Carbon core burning lasts for 600 years for a star of this size. Neon burning for 1 year, oxygen burning about 6 months (i.e. very fast on astronomical timescales)"

Clayton, Donald. Principles of Stellar Evolution and Nucleosynthesis Архивная копия от 28 августа 2017 на Wayback Machine, (1983)
http://abyss.uoregon.edu/~js/ast122/lectures/lec18.html Архивная копия от 14 февраля 2020 на Wayback Machine "Stars greater than 25 solar masses undergo a more violent end to their lives. Carbon core burning lasts for 600 years for a star of this size. Neon burning for 1 year, oxygen burning about 6 months (i.e. very fast on astronomical timescales)"