Proc. IAU volume 13, issue S334, P343-344 2017 DOI: 10.1017/s1743921317007554 View full text
J. Montalbán, A. Bressan, L. Girardi, T. Rodrigues, D. Bossini, A. Miglio, R. Scuflaire, M. Trabucchi, P. Marigo

Abstract: AbstractIn the recent years it has been generally accepted that seismic parameters add an important observational constraint for the study of stellar populations and galaxy evolution. Padova-Trieste (PARSEC) evolutionary tracks are widely used to characterise stellar objects and stellar populations. Stellar models at the base of these studies suffer from uncertainties and, more important, degeneracy among different input parameters: stellar mass, chemical composition, central chemical mixing, age, etc. Adding …

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