Detailed abundance analysis of 8 super-metal-rich star candidates

@article{Feltzing2000DetailedAA,
  title={Detailed abundance analysis of 8 super-metal-rich star candidates},
  author={S. Feltzing and Guillermo Gonzalez Lund Observatory and Sweden Astronomy Department and U. Washington and Us},
  journal={arXiv: Astrophysics},
  year={2000}
}
  • S. Feltzing, Guillermo Gonzalez Lund Observatory, +2 authors Us
  • Published 2000
  • Physics
  • arXiv: Astrophysics
  • We provide detailed abundance analyses of 8 candidate super-metal-rich stars. Five of them are confirmed to have [Fe/H] > 0.2 dex, the generally-accepted limit for super-metal-richness. Furthermore, we derive abundances of several elements and find that the stars follow trends seen in previous studies of metal-rich stars. Ages are estimated from isochrones and velocities calculated. We find that there do exist very metal-rich stars that are older than 10 Gyr. This is contrary to what is found… CONTINUE READING

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