72 citations · 116 across the 4 of their papers we have counts for
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Magnetic field morphologies in convective zones influenced by a turbulent surface layer
Anna Guseva, Ludovic Petitdemange, Charly Pinçon
Spectropolarimetric observations show that many low-mass stars possess large-scale poloidal magnetic fields with considerable dipole component, which in some cases exhibit temporal…
Thorough characterisation of the 16 Cygni system. Part II. Seismic inversions of the internal structure
G. Buldgen, M. Farnir, P. Eggenberger +5
The advent of space-based photometry observations provided high-quality asteroseismic data for a large number of stars. These observations enabled the adaptation of advanced techni…
Thorough characterisation of the 16 Cygni system Part I: Forward seismic modelling with WhoSGlAd
M. Farnir, M. -A. Dupret, G. Buldgen +5
Context: Being part of the brightest solar-like stars, and close solar analogues, the 16 Cygni system is of great interest to the scientific community and may provide insight into…
Can plume-induced internal gravity waves regulate the core rotation of subgiant stars?
C. Pinçon, K. Belkacem, M. J. Goupil +1
The seismic data provided by the satellites CoRoT and Kepler enabled us to probe the internal rotation of thousands of evolved low-mass stars. Subsequently, several studies showed…