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69:. Each process is responsible for roughly half of the observed abundances of elements heavier than
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Wallerstein, George; Icko Iben, Jr.; Peter Parker; Ann
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E. M. Burbidge; G. R. Burbidge; W. A. Fowler; F. Hoyle (1957).
100:"Synthesis of the elements in stars: forty years of progress"
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156:"Synthesis of the Elements in Stars"
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20:Neutron capture nucleosynthesis
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181:10.1103/RevModPhys.29.547
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