The Super Metal Rich Component of the Galaxyx/atl>

Details The Super Metal Rich Component of the Galaxyx/atl> The Super Metal Rich Component of the Galaxyx/atl>

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ap%26ss.265..341m&link_type=abstract

Astrophysics and Space Science, v. 265, Issue 1/4, p. 341-344 (1999).

Astronomy and Astrophysics

Astrophysics

Scientific paper

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.

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