Computer Science
Scientific paper
May 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycat..34040661b&link_type=abstract
VizieR On-line Data Catalog: J/A+A/404/661. Originally published in: 2003A&A...404..661B
Computer Science
Models: Atmosphere, Abundances: Peculiar
Scientific paper
We have computed a grid of synthetic spectra in the wavelength range λλ4600-5600Å using revised model atmospheres, for a range of atmospheric parameters and values of [alpha-elements/Fe]=0.0 and +0.4. The Lick indices Fe5270, Fe5335, Mgb and Mg2 are measured on the grid spectra, for FWHM=2 to 8.3Å. Relations between the indices Fe5270, Fe5335 and Mg2 and stellar parameters effective temperature Teff, logg, [Fe/H] and [alpha/Fe], valid in the range 4000K>=Teff>=7000K, are presented. These fitting functions are given for FWHM=3.5 and 8.3Å. The indices were also measured for a list of 97 reference stars with well-known stellar parameters observed at ESO and OHP, and these are compared to the computed indices. Finally, a comparison of the indices measured on the observed spectra and those derived from the fitting functions based on synthetic spectra is presented.
(11 data files).
Barbuy Batriz
Cayrel Roger
Coelho Paula
Katz Daniel
Perrin M.-N.
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