TiO Bands in Composite Systems

  • A. Milone
  • B. Barbuy
Conference paper
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUS, volume 153)

Abstract

TiO bands at ⋋ 620 nm are synthesized. The behaviour of these bands as a function df stellar parameters is studied. Application to composite spectra of one galactic bulge globular cluster and to bulges of elliptical. galaxies is also carried out. TiO bands may be useful metallicity indicators.

References

  1. Barbuy B.:1989, Ap&SS, 157, 111Google Scholar
  2. Barbuy B., Castro S., Ortolani, S., Bica, E.:1992a, A&A, 259, 607ADSGoogle Scholar
  3. Barbuy B., Erdelyi-Mendes M., Milone A.:1992b, A&AS, 93, 235ADSGoogle Scholar
  4. Bell R.A., Eriksson K., Gustafsson B., Nordlund A.:1976, A&AS, 23, 37ADSGoogle Scholar
  5. Bica E., Alloin D.:1986, A&A, 162, 21ADSGoogle Scholar
  6. Bica, E.:1988, A&A, 195, 76Google Scholar
  7. Davis S.P., Phillips J.G.:1963, “The Red System of CN Molecule” University of California Press, BerkeleyGoogle Scholar
  8. Kovacs, I.: 1969, “Rotational. Structure in the Spectra of Diatomic Molecules” Adam Helger Ed., LondonGoogle Scholar
  9. Moore C.E., Minnaert M.G., Houtgast J.: 1966, NBS Monograph n° 61, WashingtonGoogle Scholar
  10. Phillips J.G., Davis S.P.:1968, “The Swan System of the C2 Molecule” University of California Press, BerkeleyGoogle Scholar
  11. de Souza R.E., Barbuy B., dos Anjos S.:1992, AJ (submitted)Google Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1993

Authors and Affiliations

  • A. Milone
    • 1
  • B. Barbuy
    • 1
  1. 1.IAG-USPSão PauloBrazil

Personalised recommendations