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The evolution of the internal rotation of solar-type stars
Published online by Cambridge University Press: 18 February 2014
Abstract
We discuss the potential of asteroseismic inversion to study the internal dynamics of solar-type stars and to reconstruct the evolution of the internal rotation from the main sequence to the red-giant phase. In particular, we consider the use of gravity and mixed modes and the application of different inversion methods.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 9 , Symposium S301: Precision Asteroseismology , August 2013 , pp. 345 - 348
- Copyright
- Copyright © International Astronomical Union 2014