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Transport of angular momentum in solar-like oscillating stars
Published online by Cambridge University Press: 18 February 2014
Abstract
Our current understanding and modeling of angular momentum transport in low-mass stars are briefly reviewed. Emphasis is set on single stars slightly younger that the Sun and on subgiants and red giants observed by the space missions CoRoT and Kepler.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 9 , Symposium S301: Precision Asteroseismology , August 2013 , pp. 161 - 168
- Copyright
- Copyright © International Astronomical Union 2014
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