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High resolution measurements of galactic cosmic-ray neon, magnesium, and silicon isotopes

Journal Article · · Astrophys. J., Lett. Ed.; (United States)
DOI:https://doi.org/10.1086/183166· OSTI ID:5536247
The individual isotopes of galactic cosmic-ray Ne, Mg, and Si at approx.100 MeV per nucleon have been clearly resolved with an rms mass resolution of approx.0.20 amu. Our results suggest that the cosmic-ray source is enriched in /sup 22/Ne, /sup 25/Mg, and /sup 26/Mg when compared to the solar system. In particular, we find (/sup 25/Mg+/sup 26/Mg)//sup 24/Mg=0.49(+0.23, -0.14) compared with the solar system value of 0.27, suggesting that the cosmic-ray source and solar system material were synthesized under different conditions.
Research Organization:
California Institute of Technology
OSTI ID:
5536247
Journal Information:
Astrophys. J., Lett. Ed.; (United States), Journal Name: Astrophys. J., Lett. Ed.; (United States) Vol. 235:2; ISSN AJLEA
Country of Publication:
United States
Language:
English

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