351 citations · 5.6k across the 134 of their papers we have counts for
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Diagnoses to unravel secular hydrodynamical processes in rotating main sequence stars
T. Decressin, S. Mathis, A. Palacios +4
(Abridged) We present a detailed analysis of the main physical processes responsible for the transport of angular momentum and chemical species in the radiative regions of rotating…
Is it necessary to go beyond the ponctual mass approximation for tidal perturber in close systems?
Stephane Mathis, Christophe Le Poncin-lafitte
With the discoveries of very close star-planet systems with planet orbiting sometimes at several star radius but also with well-known situations in our solar system where natural s…
Tidal dynamics of extended bodies in planetary systems and multiple stars
Stephane Mathis, Christophe Le Poncin-Lafitte
With the discovery during the past decade of a large number of extrasolar planets orbiting their parent stars at a distance lower than 0.1 astronomical unit (and the launch and the…
Transport and mixing by internal waves in stellar interiors: effect of the Coriolis force
S. Mathis, J. -P. Zahn
We briefly recall the physical background of the transport of angular momentum and the mixing of chemicals inside stellar radiation zones and its importance for stellar evolution.…
Advances in secular magnetohydrodynamics of stellar interiors dedicated to asteroseismic spatial missions
S. Mathis, P. Eggenberger, T. Decressin +5
With the first light of COROT, the preparation of KEPLER and the future helioseismology spatial projects such as GOLF-NG, a coherent picture of the evolution of rotating stars from…
The magnetism of the solar interior for a complete MHD solar vision
S. Turck-Chieze, T. Appourchaux, J. Ballot +37
The solar magnetism is no more considered as a purely superficial phenomenon. The SoHO community has shown that the length of the solar cycle depends on the transition region betwe…