Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012cemw.confe..29f&link_type=abstract
Electronic Proceedings of "The Chemical Evolution of the Milky Way" January 23 - 27, 2012 Sexten Center for Astrophysics (SCfA).
Astronomy and Astrophysics
Astrophysics
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.
Chavez Miguel
di Marcantonio Paolo
Franchini Mariagrazia
Malagnini Maria Lucia
Morossi Carlo
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