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Oxygen-burning process : ウィキペディア英語版 | Oxygen-burning process
The oxygen-burning process is a set of nuclear fusion reactions that take place in massive stars that have used up the lighter elements in their cores. It occurs at temperatures around 1.5×109 K / 130 keV and densities of 1010 kg/m3. The principal reactions are:〔Clayton, Donald. (''Principles of Stellar Evolution and Nucleosynthesis'' ), (1983)〕
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