activity
20122022
most citedAngular momentum transport and large eddy simulations in magnetorotational turbulence: the small Pm limit

44 citations · 87 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.IM2022

Well-being in French Astrophysics

N. A. Webb, C. Bot, S. Charpinet +8

It has become clear that early career astrophysics researchers (doctoral researchers, post-docs, etc) have a very diverse appreciation of their career, with some declaring it the b…

astro-ph.EP2021

Vortex-like kinematic signal, spirals, and beam smearing effect in the HD 142527 disk

Y. Boehler, F. Ménard, C. M. T. Robert +8

Vortices are one of the most promising mechanisms to locally concentrate millimeter dust grains and allow the formation of planetesimals through gravitational collapse. The outer d…

astro-ph.SR202043 cited

The asymmetric inner disk of the Herbig Ae star HD 163296 in the eyes of VLTI/MATISSE: evidence for a vortex?

J. Varga, M. Hogerheijde, R. van Boekel +133

Context. The inner few au region of planet-forming disks is a complex environment. High angular resolution observations have a key role in understanding the disk structure and the…

astro-ph.EP2020

SPHERE+: Imaging young Jupiters down to the snowline

A. Boccaletti, G. Chauvin, D. Mouillet +130

SPHERE (Beuzit et al,. 2019) has now been in operation at the VLT for more than 5 years, demonstrating a high level of performance. SPHERE has produced outstanding results using a…

astro-ph.EP2016

Gaps, rings, and non-axisymmetric structures in protoplanetary disks - Emission from large grains

J. P. Ruge, M. Flock, S. Wolf +5

Dust grains with sizes around (sub)mm are expected to couple only weakly to the gas motion in regions beyond 10 au of circumstellar disks. In this work, we investigate the influenc…

astro-ph.SR201544 cited

Angular momentum transport and large eddy simulations in magnetorotational turbulence: the small Pm limit

H. Meheut, S. Fromang, G. Lesur +2

Angular momentum transport in accretion discs is often believed to be due to magnetohydrodynamic turbulence mediated by the magnetorotational instability. Despite an abundant liter…