Published 1981
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Implications of Ultraheavy Cosmic-Ray Source Composition Derived from Observations by the HEAO-3 Heavy Nuclei Experiment
Abstract
We have derived the contribution of r-process and s-process nucleosynthesis to the Cameron (1980) solar system (SS) abundances for Z~33. In the interval 34 ~Zs; 40 our HEA0-3 data extrapolated to the cosmic-ray source (CRS) fit the solar system mix better than r-process. In the interval 26 < Z < 40 the HEA0-3 results for CRS/SS follow the same general correlation with first ionization potential as for the lighter eiements although there are deviations in detail.
Additional Information
© IUPAP. Provided by the NASA Astrophysics Data System. This research was supported in part by NASA under contracts NPSB-27976,77,78 and grants NGR 05-002-160, 24-005-050, and 26-008-001 Space Radiation Laboratory SRL ID #: 1981-11Attached Files
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Additional details
- Eprint ID
- 45031
- Resolver ID
- CaltechAUTHORS:20140417-151643116
- NAS8-27976
- NASA
- NAS8-27977
- NASA
- NAS8-27978
- NASA
- NGR 05-002-160
- NASA
- 24-005-050
- NASA
- 26-008-001
- NASA
- Created
-
2014-04-22Created from EPrint's datestamp field
- Updated
-
2020-03-09Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 1981-11