Stellar parameters, ages and distances in F,G,K stars from spectra analysis via Lick/SDSS indices

Astronomy and Astrophysics – Astrophysics

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Galaxy: Stellar Content, Stars: Abundances, Stars: Fundamental Parameters, Stars: Late-Type

Scientific paper

Examples of stellar parameter, age, and distance estimates from spectra analyses based on comparison of observed and synthetic spectral indices are presented. We use the new synthetic library of spectral feature indices, Lick/SDSS, computed from "ad hoc" synthetic spectra to fully exploit the content of the spectroscopic SDSS-DR7 stellar database. This system is well suited to derive homogeneous and self-consistent estimates of atmospheric parameter values, Teff , log g, [Fe/H], and to study alpha-element abundances in F, G, and K stars. Then, spectroscopic distances and ages can be obtained via a Bayesian approach by using theoretical isochrones. Eventually, hints on the membership of each stars to one of the different Galactic components can be derived by studing its galactic stellar orbit using the Galactic potential by Johnston et al. (1996). In this way we attempt to take into account possible stellar migration in order to evaluate the difference between current and birthplace positions.

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