
TL;DR
This review explores the structure and evolution of the Milky Way galaxy, emphasizing the role of asteroseismology in understanding its components and future surveys in Galactic archaeology.
Contribution
It provides a comprehensive overview of Galactic components and discusses how asteroseismology and upcoming surveys advance our understanding of the Milky Way's evolution.
Findings
Asteroseismology offers new insights into Galactic structure.
Upcoming surveys like HERMES will enhance chemical tagging.
The review synthesizes current knowledge of Galactic components.
Abstract
This review discusses the structure and evolution of the Milky Way, in the context of opportunities provided by asteroseismology of red giants. The review is structured according to the main Galactic components: the thin disk, thick disk, stellar halo, and the Galactic bar/bulge. The review concludes with an overview of Galactic archaeology and chemical tagging, and a brief account of the upcoming HERMES survey with the AAT.
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