The Light Elements Be and B as Stellar Chronometers in the Early Galaxy

@article{Beers2000TheLE,
  title={The Light Elements Be and B as Stellar Chronometers in the Early Galaxy},
  author={Timothy C. Beers and Takeru K. Suzuki and Yuzuru Yoshii},
  journal={arXiv: Astrophysics},
  year={2000}
}
Recent detailed simulations of Galactic Chemical Evolution have shown that the heavy elements, in particular [Fe/H], are expected to exhibit a weak, or absent, correlation with stellar ages in the early Galaxy due to the lack of efficient mixing of interstellar material enriched by individual Type II supernovae. A promising alternative "chronometer" of stellar ages is suggested, based on the expectation that the light elements Be and B are formed primarily as spallation products of Galactic… 

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The First Stars, Proceedings of the Second MPA/ESO Workshop
  • The First Stars, Proceedings of the Second MPA/ESO Workshop
  • 2000
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