The evolution of the internal rotation of solar-type stars

The evolution of the internal rotation of solar-type stars

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 differe...

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Bibliographic Details
Published in:Proceedings of the International Astronomical Union 2013-08, Vol.9 (S301), p.345-348
Main Authors: Di Mauro, Maria Pia, Ventura, Rita, Cardini, Daniela, Christensen-Dalsgaard, Jørgen, Dziembowski, Wojciech A., Paternò, Lucio
Format: Article
Language:eng
Subjects:
Astronomy
Astrophysics
Contributed Papers
Star & galaxy formation
Stars & galaxies
Sun
Online Access:Get full text
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Summary: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.
ISSN:1743-9213
1743-9221