41 citations · 160 across the 11 of their papers we have counts for
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Tidal Dissipation in Evolved Low and Intermediate Mass Stars
M. Esseldeurs, S. Mathis, L. Decin
As the observed occurrence for planets or stellar companions orbiting low and intermediate-mass evolved stars is increasing, so does the importance of understanding and evaluating…
Testing tidal theory for evolved stars by using red-giant binaries observed by Kepler
P. G. Beck, S. Mathis, F. Gallet +4
Tidal interaction governs the redistribution of angular momentum in close binary stars and planetary systems and determines the systems evolution towards the possible equilibrium s…
The magnetic strip(s) in the advanced phases of stellar evolution - Theoretical convective turnover timescale and Rossby number for low- and intermediate-mass stars up to the AGB at various metallicities
C. Charbonnel, T. Decressin, N. Lagarde +7
Recent spectropolarimetric observations of otherwise ordinary G, K, and M giants revealed localized magnetic strips in the HRD coincident with the regions where the first dredge-up…
Tidal inertial waves in the differentially rotating convective envelopes of low-mass stars - I. Free oscillation modes
M. Guenel, C. Baruteau, S. Mathis +1
Star-planet tidal interactions may result in the excitation of inertial waves in the convective region of stars. In low-mass stars, their dissipation plays a prominent role in the…
Free inertial modes in differentially rotating convective envelopes of low-mass stars : numerical exploration
M. Guenel, C. Baruteau, S. Mathis +1
Tidally-excited inertial waves in stellar convective regions are a key mechanism for tidal dissipation in stars and therefore the evolution of close-in binary or planetary systems.…
Inertial waves in differentially rotating low-mass stars and tides
M. Guenel, C. Baruteau, S. Mathis +1
Star-planet tidal interactions may result in the excitation of inertial waves in the convective region of stars. Their dissipation plays a prominent role in the long-term orbital e…
The dynamics of the radiative zone of the Sun
S Turck-Chieze, S Couvidat, V Duez +4
Helioseismology puts strong constraints on the internal sound speed and on the rotation profile in the radiative zone. Young stars of solar type are more active and faster rotators…