The mechanisms behind the production of the heavier elements (the s- and r-processes) were first pointed out in a long theoretical paper published in 1957: ‘Synthesis of the elements in stars’ (Burbidge et al., 1957).
This revolutionary and still up-to-date paper is signed B2HF – not a strange chemical compound but the initials of the surnames of the scientists who wrote it: Margaret Burbidge, Geoffrey Burbidge, William Fowler and Fred Hoyle.
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