220 citations · 449 across the 7 of their papers we have counts for
11 papers
The magnetic obliquity of accreting T Tauri stars
Pauline McGinnis, Jérôme Bouvier, Florian Gallet
Classical T Tauri stars (CTTS) accrete material from their discs through their magnetospheres. The geometry of the accretion flow strongly depends on the magnetic obliquity, i.e.,…
Rotational evolution of solar-type protostars during the star-disk interaction phase
Florian Gallet, Claudio Zanni, Louis Amard
The early pre-main sequence phase during which they are still likely surrounded by an accretion disk represents a puzzling stage of the rotational evolution of solar-mass stars. Wh…
Star-planet tidal interaction and the limits of gyrochronology
Florian Gallet, Philippe Delorme
Age estimation techniques such as gyrochronology and magnetochronology can't be applied to stars that exchanged angular momentum with their close environment. This is especially tr…
Does magnetic field modify tidal dynamics in the convective envelope of Solar mass stars?
Aurélie Astoul, Stéphane Mathis, Clément Baruteau +5
The energy dissipation of wave-like tidal flows in the convective envelope of low-mass stars is one of the key physical mechanisms that shape the orbital and rotational dynamics of…
The magnetic fields of intermediate-mass T Tauri stars : I. Magnetic detections and fundamental stellar parameters
Florent Villebrun, Evelyne Alecian, Gaitee Hussain +13
Context. The origin of the fossil magnetic fields detected in 5 to 10% of intermediate-mass main sequence stars is still highly debated. Aims. We want to bring observational constr…
The limit of the gyrochronology - A new age determination technique: the tidal-chronology
Florian Gallet, Philippe Delorme
While the number of detected planets is continuously increasing since 1995, their impact on their central star still remain poorly understood. Yet, the presence of a massive close-…