Yields from low metallicity, intermediate mass AGB stars:. Their role for the CNO and lithium abundances in Globular Cluster stars

@article{Ventura2002YieldsFL,
  title={Yields from low metallicity, intermediate mass AGB stars:. Their role for the CNO and lithium abundances in Globular Cluster stars},
  author={P. Ventura and F. D'antona and I. Mazzitelli},
  journal={Astronomy and Astrophysics},
  year={2002},
  volume={393},
  pages={215-223}
}
  • P. Ventura, F. D'antona, I. Mazzitelli
  • Published 2002
  • Physics
  • Astronomy and Astrophysics
  • We present the results of extensive computation of the Thermal Pulse phase AGB evolution of stars of metallicities in mass fraction 2 10 4 Z 0:01, for those masses in the range 2:5 M=M 6, which suer the Hot Bottom Burning (HBB) phase. The evolution is fully computed, by assuming a mass loss rate consistent with the observations of the Magellanic Clouds lithium-rich stars, and modelling convection with the Full Spectrum of Turbulence model by Canuto and Mazzitelli. The results are discussed in… CONTINUE READING
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