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The Rotation of the Solar Radiative zone
Published online by Cambridge University Press: 01 April 2008
Abstract
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Dynamical processes are progressively introduced in stellar evolution. In this framework, the Sun is a very specific case where both models and observations have been developed in parallel during the last decade in order to progress on our present insight of solar like stars. In this poster I show the recent progress done on both sides for the rotation of the radiative zone. The present knowledge of the solar rotation profile comes from the detection of acoustic and gravity modes with the instruments GOLF and MDI aboard SoHO. In parallel we study the sensitivity of the theoretical rotation profiles obtained with the CESAM code using different rotation history in the premainsequence.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 4 , Symposium S252: The Art of Modeling Stars in the 21st Century , April 2008 , pp. 257 - 258
- Copyright
- Copyright © International Astronomical Union 2008
References
Garcia, R. A., Turck-Chieze, S., Jimenez-Reyes, S. J. et al. 2007, Science, 316, 1537CrossRefGoogle Scholar
Turck-Chieze, S., Garca, R. A., Couvidat, S. et al. 2004, ApJ 604, 455; erratum ApJ, 604, 455CrossRefGoogle Scholar
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