activity
20032026
most citedA comparative study of disc-planet interaction

446 citations · 2.4k across the 44 of their papers we have counts for

collaborators

44 papers

astro-ph.EP2026

Streaming instabilities in weakly ionized protoplanetary discs: the Ambipolar Streaming Instability (AmSI)

Arnaud Pierens, Min-Kai Lin

The regions of protoplanetary discs where planets can form are believed to be weakly ionised, suggesting thereby that non-ideal magneto-hydrodynamics (MHD) effects play an importan…

astro-ph.EP2025

Coexistence of coagulation and streaming instabilities in protoplanetary discs

Arnaud Pierens, Thomas Collin-Dufresne, Min-Kai Lin +1

The streaming instability is considered one of the leading candidates for the formation of planetesimals, due to its ability to overcome the bouncing and fragmentation barriers. Th…

astro-ph.EP2024

Thermal structure of circumbinary discs: Circumbinary planets should be icy not rocky

Arnaud Pierens, Richard P. Nelson

The process of forming a circumbinary planet is thought to be intimately related to the structure of the nascent circumbinary disc. It has been shown that the structure of a circum…

astro-ph.EP2024★ 1 cited

On the growth and evolution of low-mass planets in pressure bumps

Arnaud Pierens, Sean N. Raymond

Observations of protoplanetary discs have revealed dust rings which are likely due to the presence of pressure bumps in the disc. Because these structures tend to trap drifting peb…

astro-ph.EP2022★ 6 cited

Three-dimensional evolution of radiative circumbinary discs: the size and shape of the inner cavity

Arnaud Pierens, Richard Nelson

The evolution of circumbinary discs and planets is often studied using two-dimensional (2D) numerical simulations, although recent work suggests that 3D effects may significantly a…

astro-ph.EP2022★ 6 cited

On the evolution of pebble-accreting planets in evolving protoplanetary discs

Arnaud Pierens

We examine the migration of luminous low-mass cores in laminar protoplanetary discs where accretion occurs mainly because of disc winds and where the planet luminosity is generated…