The Super Metal Rich Component of the Galaxyx/atl> |
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| Authors: | M.L. Malagnini C. Morossi A. Buzzoni M. Chávez |
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| Affiliation: | (1) Dipartimento di Astronomia, Università degli Studi di Trieste, Via Tiepolo 11, I-34131 Trieste, Italy;(2) Osservatorio Astronomico di Trieste, Via G.B. Tiepolo, 11, I-34131 Trieste, Italy;(3) Osservatorio Astronomico di Brera, Via Brera, 28, I-20121 Milano, Italy;(4) Instituto Nacional de Astrofísica, Optica y Electrónica, CP 72000, Puebla, Mexico |
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| 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. |
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