Detailed Analysis of Nearby Bulgelike Dwarf Stars. II. Lithium Abundances

@article{Pompia2002DetailedAO,
  title={Detailed Analysis of Nearby Bulgelike Dwarf Stars. II. Lithium Abundances},
  author={Luciana Pomp{\'e}ia and Beatriz Barbuy and Michel Grenon and Bruno V Castilho},
  journal={The Astrophysical Journal},
  year={2002},
  volume={570},
  pages={820-824}
}
Li abundances are derived for a sample of bulgelike stars with isochronal ages of 10-11 Gyr. These stars have orbits with pericentric distances, Rp, as small as 2-3 kpc and Zmax < 1 kpc. The sample comprises G and K dwarf stars in the metallicity range -0.80 ≤ [Fe/H] ≤ +0.40. Few data on Li abundances in old turnoff stars (≥4.5 Gyr) within the present metallicity range are available. M67 (4.7 Gyr) and NGC 188 (6 Gyr) are the oldest studied metal-rich open clusters with late-type stars. Li… 

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