activity
19962013
most citedInfluence of gravity waves on the internal rotation and Li abundance of solar-type stars

379 citations · 2.3k across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.SR2013★ 51 cited

Impact of internal gravity waves on the rotation profile inside pre-main sequence low-mass stars

C. Charbonnel, T. Decressin, L. Amard +2

We study the impact of internal gravity waves (IGW), meridional circulation, shear turbulence, and stellar contraction on the internal rotation profile and surface velocity evoluti…

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.SR2010★ 72 cited

Effects of rotational mixing on the asteroseismic properties of solar-type stars

P. Eggenberger, G. Meynet, A. Maeder +6

The influence of rotational mixing on the evolution and asteroseismic properties of solar-type stars is studied. Rotational mixing changes the global properties of a solar-type sta…

astro-ph.SR2009★ 71 cited

Solar-like oscillations in a massive star

K. Belkacem, R. Samadi, M. -J. Goupil +15

Seismology of stars provides insight into the physical mechanisms taking place in their interior, with modes of oscillation probing different layers. Low-amplitude acoustic oscilla…

astro-ph2008★ 130 cited

Diagnoses to unravel secular hydrodynamical processes in rotating main sequence stars

T. Decressin, S. Mathis, A. Palacios +4

(Abridged) We present a detailed analysis of the main physical processes responsible for the transport of angular momentum and chemical species in the radiative regions of rotating…

astro-ph2008★ 17 cited

Deep inside low-mass stars

Corinne Charbonnel, Suzanne Talon

Low-mass stars exhibit, at all stages of their evolution, the signatures of complex physical processes that require challenging modeling beyond standard stellar theory. In this rev…