activity
20042023
most citedSeismic constraints on the radial dependence of the internal rotation profiles of six Kepler subgiants and young red giants

351 citations · 5.6k across the 134 of their papers we have counts for

collaborators
Showing 2015Show all

12 papers · 1 filter

astro-ph.SR2015★ 232 cited

The MiMeS Survey of Magnetism in Massive Stars: Introduction and overview

G. A. Wade, C. Neiner, E. Alecian +47

The MiMeS project is a large-scale, high resolution, sensitive spectropolarimetric investigation of the magnetic properties of O and early B type stars. Initiated in 2008 and compl…

astro-ph.EP2015★ 197 cited

New constraints on Saturn's interior from Cassini astrometric data

Valéry Lainey, Robert A. Jacobson, Radwan Tajeddine +15

Using astrometric observations spanning more than a century and including a large set of Cassini data, we determine Saturn's tidal parameters through their current effects on the o…

astro-ph.SR2015★ 2 cited

The variation of the tidal quality factor of convective envelopes of rotating low-mass stars along their evolution

S. Mathis

More than 1500 exoplanets have been discovered around a large diversity of host stars (from M- to A-type stars). Tidal dissipation in their convective envelope is a key actor that…

astro-ph.SR2015★ 94 cited

Rotation periods and seismic ages of KOIs - comparison with stars without detected planets from Kepler observations

T. Ceillier, J. van Saders, R. A. Garcia +7

One of the most difficult properties to derive for stars is their age. For cool main-sequence stars, gyrochronology relations can be used to infer stellar ages from measured rotati…

astro-ph.EP2015★ 5 cited

Melting the core of giant planets: impact on tidal dissipation

S. Mathis

Giant planets are believed to host central dense rocky/icy cores that are key actors in the core-accretion scenario for their formation. In the same time, some of their components…

astro-ph.EP2015

Scaling laws to quantify tidal dissipation in star-planet systems

Pierre Auclair-Desrotour, Stéphane Mathis, Christophe Le Poncin-Lafitte

Planetary systems evolve over secular time scales. One of the key mechanisms that drive this evolution is tidal dissipation. Submitted to tides, stellar and planetary fluid layers…