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| | Astron. Astrophys. 337, 714-720 (1998) |
 | | In the 70's and 80's the problem of Li, Be and B (hereafter LiBeB) nucleosynthesis has been considered essentially solved by Galactic Cosmic Ray (GCR) spallation (Meneguzzi, Audouze and Reeves 1971, Reeves 1994). |
 | | First, as we noted above, if the cosmic rays are accelerated out of the ISM and interact in the ISM, the rising CNO/H abundance in the ISM leads to cumulative Be and B abundances which depend quadratically on the ISM metallicity, and thus is in disagreement with the observations. |
 | | If the Be in the early Galaxy is indeed produced by particles whose acceleration is related to short-lived very massive stars, then the difference in the lifetimes of the progenitors of Be and Fe and the relative number of stars implied in each case, could also affect the evolution of Be/Fe. |
| aa.springer.de /papers/8337003/2300714/sc1.htm (1405 words) |
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