Deep inside low-mass stars

Details Deep inside low-mass stars Deep inside low-mass stars

2008-05-30

arxiv.org/abs/0805.4697v1

Astronomy and Astrophysics

Astrophysics

Invited Review to be published in the proceedings of the IAU Symposium 252 "The Art of Modelling stars in the 21st Century" -

Scientific paper

10.1017/S1743921308022710

Low-mass stars exhibit, at all stages of their evolution, the signatures of complex physical processes that require challenging modeling beyond standard stellar theory. In this review, we recall the most striking observational evidences that probe the interaction and interdependence of various transport processes of chemicals and angular momentum in these objects. We then focus on the impact of atomic diffusion, large scale mixing due to rotation, and internal gravity waves on stellar properties on the main sequence and slightly beyond.

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