• DOI:10.1051/0004-6361:20021001
Corpus ID: 14404796

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

View via Publisher

aanda.org

Save to Library

Create Alert

Cite

Launch Research Feed