37 citations · 94 across the 14 of their papers we have counts for
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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…
Gravito-inertial waves in a differentially rotating spherical shell
Giovanni M. Mirouh, Clément Baruteau, Michel Rieutord +1
The gravito-inertial waves propagating over a shellular baroclinic flow inside a rotating spherical shell are analysed using the Boussinesq approximation. The wave properties are e…
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.…
Gravito-inertial modes in a differentially rotating spherical shell
Giovanni M. Mirouh, Clément Baruteau, Michel Rieutord +1
While many intermediate- and high-mass main sequence stars are rapidly and differentially rotating, the effects of rotation on oscillation modes are poorly known. In this communica…
Gravito-inertial modes in a differentially rotating spherical shell
Giovanni M. Mirouh, Clément Baruteau, Michel Rieutord +1
Oscillations have been detected in a variety of stars, including intermediate- and high-mass main sequence stars. While many of these stars are rapidly and differentially rotating,…
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…