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http://hdl.handle.net/20.500.12386/33174| Title: | The Super Metal Rich Component of the Galaxyx | Authors: | Malagnini, M. L. MOROSSI, Carlo BUZZONI, Alberto Chávez, M. |
Issue Date: | 1999 | Journal: | ASTROPHYSICS AND SPACE SCIENCE | Number: | 265 | Issue: | 1/4 | First Page: | 341 | 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. | URI: | http://hdl.handle.net/20.500.12386/33174 | URL: | https://link.springer.com/article/10.1023/A:1002140700934 | ISSN: | 0004-640X | DOI: | 10.1023/A:1002140700934 | Bibcode ADS: | 1999Ap&SS.265..341M | Fulltext: | open |
| Appears in Collections: | 1.01 Articoli in rivista |
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| File | Description | Size | Format | |
|---|---|---|---|---|
| A_1002140700934.pdf | postprint | 35.15 kB | Adobe PDF | View/Open |
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