The Super Metal Rich Component of the Galaxyx/atl>
Abstract
We present the results obtained by comparing mid-resolution stellar spectra of super metal rich candidates with synthetic spectra computed in the wavelength range 4850-5400 Å. Atmospheric parameters, derived by using the flux fitting method, are illustrated for a sample of representative stars. The final aim of the project is the definition of a fully consistent metallicity scale for SMR stars.
- Publication:
-
Astrophysics and Space Science
- Pub Date:
- July 1999
- DOI:
- 10.1023/A:1002140700934
- Bibcode:
- 1999Ap&SS.265..341M