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    Beryllium and Boron abundances in population II stars (1995)
    In:  CASI
    Details
    Publication Date: 2019-06-28
    Description: The scientific focus of this program was to undertake UV spectroscopic abundance analyses of extremely metal poor stars with attention to determining abundances of light elements such as beryllium and boron. The abundances are likely to reflect primordial abundances within the early galaxy and help to constrain models for early galactic nucleosynthesis. The general metal abundances of these stars are also important for understanding stellar evolution.
    Keywords: ASTROPHYSICS
    Type: NASA-CR-189434 , NAS 1.26:189434 , RHPU-0429
    Format: application/pdf
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