ATTENZIONE!!! IL SISTEMA E' UTILIZZABILE ESCLUSIVAMENTE IN MODALITA' "CONSULTAZIONE". CAUSA PROBLEMI TECNICI, SI PREGA DI NON EFFETTUARE L'AUTENTICAZIONE, FINO A NUOVA COMUNICAZIONE. GRAZIE
 

The Super Metal Rich Component of the Galaxyx

Journal
Date Issued
1999
Author(s)
Malagnini, M. L.
•
•
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Chávez, M.
DOI
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.
Volume
265
Issue
1/4
Start page
341
Uri
Url
Issn Identifier
0004-640X
Ads BibCode
1999Ap&SS.265..341M
Rights
open.access
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