K. Pouilly
University of Grenoble
11 Papers
15 Citations
K. Pouilly is an academic researcher from University of Grenoble. The author has contributed to research in topics: Accretion (astrophysics) & Light curve. The author has an hindex of 4, co-authored 5 publications.
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Papers
Magnetospheric accretion in the intermediate-mass T Tauri star HQ Tauri
K. Pouilly,Jerome Bouvier,Evelyne Alecian,S. H. P. Alencar,Ann Marie Cody,Jean-François Donati,K. N. Grankin,G. A. J. Hussain,L. M. Rebull,Colin P. Folsom +9 more
TL;DR: In this paper, the authors investigate the accretion process in the young stellar system HQ Tau, an intermediate-mass T Tauri star (1.9 M ) and report HQ Tau to be a spectroscopic binary candidate whose orbit remains to be determined.
Investigating the magnetospheric accretion process in the young pre-transitional disk system DoAr 44 (V2062 Oph). A multiwavelength interferometric, spectropolarimetric, and photometric observing campaign
Jerome Bouvier,Evelyne Alecian,S. H. P. Alencar,A. P. Sousa,Jean-François Donati,Karine Perraut,Amelia Bayo,L. M. Rebull,Catherine Dougados,Gilles Duvert,Jean-Phillipe Berger,Myriam Benisty,Myriam Benisty,K. Pouilly,Colin P. Folsom,C. Moutou +15 more
TL;DR: In this article, the magnetospheric accretion/ejection process in the young stellar system DoAr 44 (V2062 Oph) was investigated using high-resolution spectropolarimetry at both optical and near-IR wavelengths with long-baseline near IR inteferometry and multicolor photometry.
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,Evelyne Alecian,S. H. P. Alencar,A. P. Sousa,J.-F. Donati,K. Perraut,Amelia Bayo,L. M. Rebull,Catherine Dougados,Gilles Duvert,J. P. Berger,Myriam Benisty,K. Pouilly,C. P. Folsom,C. Moutou +14 more
TL;DR: In this article, the magnetospheric accretion process in the young stellar system DoAr 44 is investigated, and it is shown that the magnetic field is strong enough to disrupt the inner disk close to the corotation radius, at a distance of about 4.6 stellar radii.
Magnetospheric accretion in the intermediate-mass T Tauri star HQ Tau
K. Pouilly,J. Bouvier,Evelyne Alecian,S. H. P. Alencar,Ann Marie Cody,J.-F. Donati,K. N. Grankin,G. A. J. Hussain,L. M. Rebull,C. P. Folsom +9 more
TL;DR: In this paper, the authors investigate the accretion process in the young stellar system HQ Tau, an intermediate-mass T Tauri star (1.9 M ) and report HQ Tau to be a spectroscopic binary candidate whose orbit remains to be determined.
Stable accretion and episodic outflows in the young transition disk system GM Aurigae. A semester-long optical and near-infrared spectrophotometric monitoring campaign
Jerome Bouvier,A. P. Sousa,K. Pouilly,J. M. Almenara,J.-F. Donati,S. H. P. Alencar,A. Frasca,K. N. Grankin,Andres Carmona,George Pantolmos,B. Zaire,Xavier Bonfils,A. Bay,Luisa Rebull,J. Alonso-Santiago,J. F. Gameiro,Neil Cook,Étienne Artigau,the SPIRou consortium +18 more
TL;DR: In this paper , the structure and dynamics of the magnetospheric accretion region and associated outflows on a scale smaller than 0.1 au around the young transitional disk system GM Aur were investigated.