Beryllium and Boron abundances in population II stars

Details Beryllium and Boron abundances in population II stars Beryllium and Boron abundances in population II stars

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995csc..reptr.....&link_type=abstract

Final Report Computer Sciences Corp., Calverton, MD.

Computer Science

Abundance, Beryllium, Boron, F Stars, Galactic Evolution, Metallicity, Spectroscopic Analysis, Supergiant Stars, Ultraviolet Spectra, Iue, Light Elements, Nuclear Fusion, Nuclear Reactions, Stellar Evolution

Scientific paper

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.

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