613 citations · 7.1k across the 103 of their papers we have counts for
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Investigating the magnetospheric accretion process in the young pre-transitional disk system DoAr 44 (V2062~Oph). A multiwavelength interferometric, spectropolarimetric, and photometric observing campaign
J. Bouvier, E. Alecian, S. H. P. Alencar +13
Young stars interact with their accretion disk through their strong magnetosphere. We investigate the magnetospheric accretion process in the young stellar system DoAr 44. We monit…
Reading between the lines: Disk emission, wind, and accretion during the ZCMa NW outburst
A. Sicilia-Aguilar, J. Bouvier, C. Dougados +2
(Abridged) We use optical spectroscopy to investigate the disk, wind, and accretion during the 2008 ZCMa NW outburst. Over 1000 optical emission lines reveal accretion, a variable,…
The lithium-rotation connection in young stars
J. Bouvier
Lithium is a sensitive probe to mixing processes operating in stellar interiors. For many years, a connection has been suspected to exist between lithium abundances and stellar rot…
Magnetic torques on T Tauri stars: accreting vs. non-accreting systems
G. Pantolmos, C. Zanni, J. Bouvier
Classical T Tauri stars (CTTs) magnetically interact with their surrounding disks, a process that is thought to regulate their rotational evolution. In this work, we compute torque…
Magnetospheric accretion in the intermediate-mass T Tauri star HQ Tau
K. Pouilly, J. Bouvier, E. Alecian +7
Context. Classical T Tauri stars (cTTs) are pre-main sequence stars surrounded by an accretion disk. They host a strong magnetic field, and both magnetospheric accretion and ejecti…
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.,…