The evolution of the internal rotation of solar-type stars
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.
- Publication:
-
Precision Asteroseismology
- Pub Date:
- February 2014
- DOI:
- 10.1017/S1743921313014567
- Bibcode:
- 2014IAUS..301..345D
- Keywords:
-
- stars: oscillations;
- stars: rotation;
- stars: evolution;
- Sun: helioseismology;
- Sun: evolution;
- Sun: rotation