activity
20182021
most citedSlingshot prominences: coronal structure, mass loss and spin down

23 citations · 23 across the 1 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2021

PENELLOPE: the ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES) I. Survey presentation and accretion properties of Orion OB1 and -Orionis

C. F. Manara, A. Frasca, L. Venuti +69

The evolution of young stars and disks is driven by the interplay of several processes, notably accretion and ejection of material. Critical to correctly describe the conditions of…

astro-ph.SR2020

Identifying solar-like magnetic cycles with Zeeman-Doppler-Imaging (ZDI)

Lisa T. Lehmann, Gaitee A. J. Hussain, Aline A. Vidotto +2

We are reaching the point where spectropolarimetric surveys have run for long enough to reveal solar-like magnetic activity cycles. In this paper we investigate what would be the b…

astro-ph.SR201923 cited

Slingshot prominences: coronal structure, mass loss and spin down

M. Jardine, A. Collier Cameron, J. -F. Donati +1

The structure of a star's coronal magnetic field is a fundamental property that governs the high-energy emission from the hot coronal gas and the loss of mass and angular momentum…

astro-ph.SR2018

The magnetic propeller accretion regime of LkCa 15

J-F Donati, J Bouvier, SH Alencar +12

We present a spectropolarimetric study of the classical T Tauri star (cTTS) LkCa 15 investigating the large-scale magnetic topology of the central star and the way the field connec…

astro-ph.SR2018

Inner disk structure of the classical T Tauri star LkCa 15

S. H. P. Alencar, J. Bouvier, J. -F. Donati +15

Magnetospheric accretion has been thoroughly studied in young stellar systems with full non-evolved accretion disks, but it is poorly documented for transition disk objects with la…

astro-ph.SR2018

Observing the simulations: Applying ZDI to 3D non-potential magnetic field simulations

L. T. Lehmann, G. A. J. Hussain, M. M. Jardine +2

The large-scale magnetic fields of stars can be obtained with the Zeeman-Doppler-Imaging (ZDI) technique, but their interpretation is still challenging as the contribution of the s…