activity
20062026
most citedLocal outflows from turbulent accretion disks

151 citations · 1.9k across the 82 of their papers we have counts for

collaborators

82 papers

astro-ph.CO2026

Magneto-Thermal Instability in Galaxy Clusters -- III. The Limit of Adiabatic Stratification

Lorenzo Maria Perrone, Henrik Latter

In the hot and dilute intracluster medium of galaxy clusters, large-scale buoyancy instabilities can develop due to the transport of heat along magnetic field lines. In particular,…

astro-ph.EP2026

The effect of dust on vortices II: Streaming instabilities

Nathan Magnan, Henrik Nils Latter

One of the main questions in planet formation theory is how to cross the metre-scale barrier. In this two-part series, we assess the merits of vortex-based theories by investigatin…

astro-ph.EP2026

The effect of dust on vortices I: Laminar models

Nathan Magnan, Henrik Nils Latter

One of the main questions regarding planet formation is how to cross the metre-scale barrier. Several theories rely on the formation of dust clumps dense enough to collapse under t…

astro-ph.EP2026★ 2 cited

Global magnetohydrodynamic simulations of the inner regions of protoplanetary discs. II. Vertical-net-flux regime

Matthew J. O. Roberts, Henrik N. Latter, Geoffroy Lesur

The inner regions of protoplanetary discs, which encompass the putative habitable zone, are dynamically complex, featuring a relatively well-ionised, turbulent active zone located…

astro-ph.HE2025★ 1 cited

On the numerical convergence of MRI simulations

Thomas Jannaud, Henrik N. Latter

The magnetorotational instability (MRI) plays a crucial role in the evolution of many types of accretion disks. It is often studied using ideal-MHD numerical simulations. In princi…

astro-ph.SR2025★ 2 cited

Instability and vertical eccentricity variation in global hydrodynamic disk simulations

Janosz W. Dewberry, Henrik N. Latter, Gordon I. Ogilvie +1

Many dynamical interactions can induce eccentricities in astrophysical accretion disks. Disk eccentricities in turn seed a variety of instabilities, even in ideal hydrodynamics. We…