activity
20112024
most citedThe 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

41 citations · 160 across the 11 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2024★ 12 cited

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…

astro-ph.EP2023★ 1 cited

Hydrodynamic modelling of dynamical tides dissipation in Jupiter's interior as revealed by Juno

Hachem Dhouib, Clément Baruteau, Stéphane Mathis +3

The Juno spacecraft has acquired exceptionally precise data on Jupiter's gravity field, offering invaluable insights into Jupiter's tidal response, interior structure, and dynamics…

astro-ph.EP2023

Hydrodynamical modelling of tidal dissipation in gas giant planets at the time of space missions

Hachem Dhouib, Clément Baruteau, Stéphane Mathis +3

Gas giant planets are differentially rotating magnetic objects that have strong and complex interactions with their environment. In our Solar system, they interact with their numer…

astro-ph.SR2018★ 23 cited

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…

astro-ph.SR2017★ 41 cited

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…

astro-ph.SR2016★ 37 cited

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…