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- W990561507 abstract "The mean abundance of Li in stars formed within the past 5 Gyr is log N(Li) = 3.2(±0.2) while the corresponding value for the oldest stars in the galaxy is log N(Li) = 2.2(±0.2). As long as the potential source of Li in the galactic disc cannot be identified there remains reasonable doubt about whether the latter represents the primordial Li abundance. Spallation of interstellar CNO nuclei by the 4 He and proton components of galactic cosmic rays (GCR) was proposed, over 20 years ago, as a source of Li but production falls short by an order of magnitude. Recently α + α fusion was invoked to explain some Li production in the early Galaxy, but this reaction yielded, apparently, to much Li in the old disc, or too-little Li in young stars." @default.
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- W990561507 date "1995-01-01" @default.
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- W990561507 title "Light Element Production in the Galactic Disc by Delayed Low Energy Cosmic Ray Flux from Intermediate Mass Stars" @default.
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