S-R-processes-atomic-mass-201-to-210


Autor:
Credit:
Praca własna, based on (1973). "Abundance of the Elements in the Solar System". Space Science Review 15: 121–146. DOI:10.1007/BF00172440. and
E. M. Burbidge, G. R. Burbidge, W. A. Fowler, and F. Hoyle (1957). "Synthesis of the Elements in Stars". Reviews of Modern Physics 29 (4): 547. DOI:10.1103/RevModPhys.29.547.
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źródło:
Wymiary:
440 x 340 Pixel (40335 Bytes)
Opis:
Chart representing the final part of the s-process. Red horizontal lines with a circle in their right ends represent neutron captures; blue arrows pointing up-left represent beta decays; green arrow pointing down-left represents an alpha decay; cyan arrows pointing down-right represent electron captures.
Licencja:
CC0
Warunki licencji:
Creative Commons Zero, Public Domain Dedication

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