OB Associations, Wolf–Rayet Stars, and the Origin of Galactic Cosmic Rays

@article{Binns2007OBAW,
  title={OB Associations, Wolf–Rayet Stars, and the Origin of Galactic Cosmic Rays},
  author={W. R. Binns and M. E. Wiedenbeck and Marcel Arnould and Alan C. Cummings and G. A. de Nolfo and Stephane Goriely and M. H. Israel and R. A. Leske and Richard A. Mewaldt and Georges Meynet and Lauren M. Scott and Edward C. Stone and T. T. von Rosenvinge},
  journal={Space Science Reviews},
  year={2007},
  volume={130},
  pages={439-449}
}
Abstract We have measured the isotopic abundances of neon and a number of other species in the galactic cosmic rays (GCRs) using the Cosmic Ray Isotope Spectrometer (CRIS) aboard the ACE spacecraft. Our data are compared to recent results from two-component (Wolf–Rayet material plus solar-like mixtures) Wolf–Rayet (WR) models. The three largest deviations of galactic cosmic ray isotope ratios from solar-system ratios predicted by these models, 12C/16O, 22Ne/20Ne, and 58Fe/56Fe, are very close… 

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Wolf-Rayet stars, OB associations, and the origin of galactic cosmic rays

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