Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S301(9), p. 161-168, 2013
DOI: 10.1017/s1743921313014269
Full text: Unavailable
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.