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Asteroseismology of Red Giants and Galactic Archaeology

  • Saskia HekkerEmail author
Conference paper
Part of the Astrophysics and Space Science Proceedings book series (ASSSP, volume 49)

Abstract

From the oscillations in red-giant stars measured in time-series data it is possible to derive more accurate stellar parameters (e.g., mass, radius and age) as can be done using only single-epoch spectroscopy or photometry. These stellar parameters combined with chemical composition and the position, distance and velocity of the stars play an important role in studying the formation and evolution of the Milky Way. In this chapter we discuss some key physical phenomena that are at play in (red-giant) stars as well as some important phases in red-giant evolution. Subsequently, oscillation characteristics that are of importance for the determination of stellar parameters (as indicated above) of red-giant stars are introduced followed by a description of the main components of the Milky Way. Finally, the role red giants can play in creating a detailed observational picture of the Milky Way and deciphering the formation and evolution of the Milky Way is discussed.

Notes

Acknowledgements

I would like to thank Alexey Mints, George Angelou and Maarten Mooij for useful discussions and comments on earlier versions of the manuscript. Furthermore, I acknowledge Earl Bellinger, Abishek Datta and Thomas Constantino for providing stellar evolution models used for figures. I acknowledge funding from the European Research Council under the European Community’s Seventh Framework Programme (FP7/2007–2013)/ERC grant agreement no 338251 (StellarAges).

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Copyright information

© Springer International Publishing AG 2018

Authors and Affiliations

  1. 1.Max Planck Institute for Solar System ResearchSAGE research groupGöttingenGermany
  2. 2.Department of Physics and Astronomy, Stellar Astrophysics Centre (SAC)Aarhus UniversityAarhus CDenmark

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