activity
19992026
most citedLarge-scale magnetic topologies of mid-M dwarfs

465 citations · 3.7k across the 61 of their papers we have counts for

collaborators

63 papers

astro-ph.SR2026

Transport of angular momentum and chemical elements by the MRI dynamo in stellar radiative zones

Laurène Jouve, François Lignières, Jérôme Guilet +1

The question of angular momentum transport by magnetic fields has recently been revived by the detection of magnetic fields in the deep interior of red giant stars. We aim at chara…

astro-ph.SR2025

Stable magnetic fields and changing starspots on Vega -- An ultra-deep decadal survey at Pic du Midi and OHP

T. Böhm, M. Holschneider, P. Petit +4

Monitoring magnetic and activity variations in A- and B-type stars with ultra-weak magnetic fields is essential to understand the origin and evolution of these fields in this regio…

astro-ph.SR2024★ 3 cited

Properties of observable mixed inertial and gravito-inertial modes in γ Doradus stars

Marion Galoy, François Lignières, Jérôme Ballot

In γ Doradus stars, gravito-inertial modes in the radiative zone and inertial modes in the convective core can interact resonantly, which translates into the appearance of dip stru…

astro-ph.IM2024★ 13 cited

The PLATO Mission

Heike Rauer, Conny Aerts, Juan Cabrera +842

PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…

astro-ph.SR2023★ 1 cited

Angular momentum and chemical transport by azimuthal magnetorotational instability in radiative stellar interiors

Domenico G. Meduri, Laurène Jouve, François Lignières

The transport of angular momentum (AM) and chemical elements within evolving stars remains poorly understood. Recent observations showed that the radiative cores of low mass main s…

astro-ph.SR2020★ 64 cited

First evidence of inertial modes in Doradus stars: The core rotation revealed

R-M. Ouazzani, F. Lignières, M-A. Dupret +4

Gamma Doradus stars present an incredibly rich pulsation spectra, with gravito-inertial modes, in some cases supplemented with delta Scuti-like pressure modes and in numerous cases…