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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S301(9), p. 161-168, 2013

DOI: 10.1017/s1743921313014269

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Transport of angular momentum in solar-like oscillating stars

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Data provided by SHERPA/RoMEO

Abstract

AbstractOur 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 missionsCoRoTandKepler.

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