activity
19962017
most citedSeismic diagnostics for transport of angular momentum in stars 1. Rotational splittings from the PMS to the RGB

310 citations · 3.6k across the 42 of their papers we have counts for

collaborators

42 papers

astro-ph.SR2017★ 18 cited

Confinement of the solar tachocline by a cyclic dynamo magnetic field

R. Barnabé, A. Strugarek, P. Charbonneau +2

The surprising thinness of the solar tachocline is still not understood with certainty today. Among the numerous possible scenarios suggested to explain its radial confinement, one…

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.SR2014★ 107 cited

The Magnetic Fields at the Surface of Active Single G-K Giants

M. Aurière, R. Konstantinova-Antova, C. Charbonnel +15

We investigate the magnetic field at the surface of 48 red giants selected as promising for detection of Stokes V Zeeman signatures in their spectral lines. We use the spectropolar…

astro-ph.EP2014★ 30 cited

The surface signature of the tidal dissipation of the core in a two-layer planet

F. Remus, S. Mathis, J. -P. Zahn +1

Tidal dissipation, which is directly linked to internal structure, is one of the key physical mechanisms that drive systems evolution and govern their architecture. A robust evalua…

astro-ph.SR2012★ 310 cited

Seismic diagnostics for transport of angular momentum in stars 1. Rotational splittings from the PMS to the RGB

J. P. Marques, M. J. Goupil, Y. Lebreton +12

Rotational splittings are currently measured for several main sequence stars and a large number of red giants with the space mission Kepler. This will provide stringent constraints…

astro-ph.EP2012

The anelastic equilibrium tide in exoplanetary systems

F. Remus, S. Mathis, J. -P. Zahn +1

Earth-like planets have anelastic mantles, whereas giant planets may have anelastic cores. As for the fluid parts of a body, the tidal dissipation of such solid regions, gravitatio…