Structure and Evolution of the Milky Way
arXiv:1108.5028 · doi:10.1007/978-3-642-18418-5_14
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.
Proc. of the workshop "Red Giants as Probes of the Structure and Evolution of the Milky Way" (Roma, 15-17 Nov 2010), Astrophysics and Space Science Proceedings, ISBN 978-3-642-18417-8 (eds. A. Miglio, J. Montalban, A. Noels). Part of RedGiantsMilkyWay/2011/ proceedings available at http://arxiv.org/html/1108.4406v1
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Cited by in corpus (6)
- Chemodynamical evolution of the Milky Way disk I: The solar vicinity
- Verifying asteroseismically determined parameters of Kepler stars using hipparcos parallaxes: self-consistent stellar properties and distances
- PLATO as it is: a legacy mission for Galactic archaeology
- Origin of the Metallicity Distribution in the Thick Disc
- The most ancient spiral galaxy: a 2.6-Gyr-old disk with a tranquil velocity field
- The velocity ellipsoid in the Galactic disc using Gaia DR1