Asteroseismology of Red Giants as a Tool for Studying Stellar Populations: First Steps

Abstract

The detection of solar-like oscillations in G and K giants with the CoRoT and Keplerspace-based satellites allows robust constraints to be set on the mass and radius of such stars. The availability of these constraints for thousands of giants sampling different regions of the Galaxy promises to enrich our understanding on the Milky Way’s constituents. In this contribution we briefly recall which are the relevant constraints that red-giant seismology can currently provide to the study of stellar populations. We then present, for a few nearby stars, the comparison between radius and mass determined using seismic scaling relations and those obtained by other methods.