Table of Contents of: "Asteroseismology of Stellar Populations in the Milky Way"

TL;DR

This paper provides a comprehensive overview of a workshop focused on combining asteroseismology and spectroscopy to study stellar populations in the Milky Way, highlighting recent results and future prospects.

Contribution

It compiles key discussions and results from a 2013 workshop, emphasizing the integration of seismic and spectroscopic data for Galactic evolution studies.

Findings

Integration of seismic and spectroscopic data enhances understanding of stellar populations.

First results from CoRoT and Kepler surveys demonstrate their value in Galactic studies.

Future Gaia data will further advance Milky Way research.

Abstract

We give here the Table of Contents and clickable links to papers of the proceedings from the workshop "Asteroseismology of Stellar Populations in the Milky Way", held in Sesto, 22-26 July 2013. The aim of this workshop was to foster collaborations and discussions between expert researchers in Galactic evolution, specialists in stellar structure and asteroseismology, and key representatives of extensive ground-based spectroscopic surveys such as APOGEE and the ESO-Gaia Spectroscopic Survey. The workshop was devoted to discussing first results achieved by combining spectroscopic and seismic constraints on populations of stars observed by CoRoT and Kepler, and the relevance of CoRoT and Kepler surveys in the context of future Gaia observations.