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The evolution of the internal rotation of solar-type stars

Published online by Cambridge University Press:  18 February 2014

Maria Pia Di Mauro ,
Rita Ventura ,
Daniela Cardini ,
Jørgen Christensen-Dalsgaard ,
Wojciech A. Dziembowski  and
Lucio Paternò
Maria Pia Di Mauro
Affiliation:
INAF-IAPS Istituto di Astrofisica e Planetologia Spaziali, Via del Fosso del Cavaliere 100, 00133 Roma, Italy email: maria.dimauro@inaf.it
Rita Ventura
Affiliation:
INAF-Astrophysical Observatory of Catania, Via S. Sofia 78, 95020, Catania, Italy
Daniela Cardini
Affiliation:
INAF-IAPS Istituto di Astrofisica e Planetologia Spaziali, Via del Fosso del Cavaliere 100, 00133 Roma, Italy email: maria.dimauro@inaf.it
Jørgen Christensen-Dalsgaard
Affiliation:
Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
Wojciech A. Dziembowski
Affiliation:
Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
Lucio Paternò
Affiliation:
INAF-Astrophysical Observatory of Catania, Via S. Sofia 78, 95020, Catania, Italy
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Abstract

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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

stars: oscillationsstars: rotationstars: evolutionSun: helioseismologySun: evolutionSun: rotation
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 

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