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Asteroseismology of Stellar Populations in the Milky Way

Asteroseismology of Stellar Populations in the Milky Way

Hardcover

Series: Astrophysics and Space Science Proceedings, Book 39

Astronomy & SpacePhysics

ISBN10: 3319109928
ISBN13: 9783319109923
Publisher: Springer Nature
Published: Jan 16 2015
Pages: 185
Weight: 1.01
Height: 0.50 Width: 6.14 Depth: 9.21
Language: English

The detection of radial and non-radial solar-like oscillations in thousands of G-K giants with CoRoT and Kepler is paving the road for detailed studies of stellar populations in the Galaxy. The available average seismic constraints allow largely model-independent determination of stellar radii and masses, and can be used to determine the position and age of thousands of stars in different regions of the Milky Way, and of giants belonging to open clusters. Such a close connection between stellar evolution, Galactic evolution, and asteroseismology opens a new very promising gate in our understanding of stars and galaxies.

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