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- W3201942648 abstract "The /sup 22/Ne excess at the cosmic-ray source is discussed in terms of a /sup 22/Ne-rich component injected and accelerated by carbon-rich Wolf-Rayet stars. The overabundance of /sup 22/Ne relative to /sup 20/Ne predicted at the surface of these stars is estimated to a factor approx.120 with respect to solar system abundances. In order to give rise to a /sup 22/Ne excess of about 3 at the cosmic-ray sources as inferred from observations, the carbon-rich Wolf-Rayet contribution to the primary cosmic-ray flux is to be at maximum 1/60. This component would be energized by strong stellar winds producing quasi-standing shocks around the Wolf-Rayet stars." @default.
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- W3201942648 date "1981-01-01" @default.
- W3201942648 modified "2023-09-28" @default.
- W3201942648 title "On the Stellar Origin of the NE 22 Excess in Cosmic Rays" @default.
- W3201942648 hasPublicationYear "1981" @default.
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