220 citations · 770 across the 16 of their papers we have counts for
9 papers · 1 filter
Monte-Carlo simulations of evolving rotational distributions of low-mass stars in young open clusters. Testing the influence of initial conditions
Maria Jaqueline Vasconcelos, Jérôme Bouvier, Florian Gallet +1
The rotational evolution of a young stellar population can give informations about the rotation pattern of more evolved clusters. Combined with rotational period values of thousand…
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…
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…
Magnetic fields of intermediate mass T Tauri stars
A. Lavail, O. Kochukhov, G. A. J. Hussain +3
Aims. In this paper, we aim to measure the strength of the surface magnetic fields for a sample of five intermediate mass T Tauri stars and one low mass T Tauri star from late-F to…
The impact of rotation on turbulent tidal friction in stellar and planetary convective regions
Stéphane Mathis, Pierre Auclair-Desrotour, Mathieu Guenel +2
Turbulent friction in convective regions in stars and planets is one of the key physical mechanisms that drive the dissipation of the kinetic energy of tidal flows in their interio…
Rotating models of young solar-type stars : Exploring braking laws and angular momentum transport processes
Louis Amard, Ana Palacios, Corinne Charbonnel +2
We study the predicted rotational evolution of solar-type stars from the pre-main sequence to the solar age with 1D rotating evolutionary models including physical ingredients. We…
Improved angular momentum evolution model for solar-like stars II. Exploring the mass dependence
Florian Gallet, Jérôme Bouvier
We developed angular momentum evolution models for 0.5 and 0.8 stars. The parametric models include a new wind braking law based on recent numerical simulations of magn…