Metallicities and kinematics of G and K dwarfs

@article{Flynn1997MetallicitiesAK,
  title={Metallicities and kinematics of G and K dwarfs},
  author={C. Flynn and O. Morell},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={1997},
  volume={286},
  pages={617-625}
}
  • C. Flynn, O. Morell
  • Published 1997
  • Physics
  • Monthly Notices of the Royal Astronomical Society
  • We have used accurate, spectroscopically determined abundances for G and K dwarfs of Morell, Kallander & Butcher and Morell to derive a photometric abundance index for G and K dwarfs. Broad-band Cousins R - I photometry is used to estimate effective temperature and the Geneva bi colour to estimate line blanketing in the blue and hence abundance. Abundances can be derived in the range -2.0 <[FelH]< 0.5 for GO to K3 dwarfs, with a scatter in [FelH] of 0.2 dex. We apply the method to a sample of… CONTINUE READING
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    References

    SHOWING 1-2 OF 2 REFERENCES
    Rev. Mex. Astr. Astrof
    • Rev. Mex. Astr. Astrof
    • 1989