File:S-R-processes-atomic-mass-201-to-210.svg

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Summary

Description
English: 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 decay; green arrow pointing down-left represents an alpha decay; cyan arrows pointing down-right represent electron captures.
Date
Source Own work, based on (1973). "Abundance of the Elements in the Solar System". Space Science Review 15: 121–146. DOI:10.1007/BF00172440. Archived from the original on 2011-10-21. Retrieved on 2016-03-13. 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. Archived from the original on 2016-06-24. Retrieved on 2016-03-13.
Author R8R Gtrs

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Captions

The final part of the s-process from mass numbers 201 to 210.

Items portrayed in this file

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inception

13 March 2016

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image/svg+xml

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current17:02, 28 July 2023Thumbnail for version as of 17:02, 28 July 2023440 × 340 (20 KB)Great BrightstarFix some text alignments

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