most citedDust-void evolution driven by turbulent dust flux can induce runaway migration of Earth-mass planets

3 citations · 6 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2025

The LISA Astrophysics "Disc-IMRI" Code Comparison Project: Intermediate-Mass-Ratio Binaries in AGN-Like Discs

Andrea Derdzinski, Alexander J. Dittmann, Alessia Franchini +16

Upcoming space-based gravitational wave detectors such as LISA, the Laser Interferometer Space Antenna, will be sensitive to extreme- and intermediate-mass-ratio inspirals (EMRIs a…

astro-ph.EP2025

The reflex instability: exponential growth of a large-scale mode in astrophysical discs

Aurélien Crida, Clément Baruteau, Jean-François Gonzalez +5

We report the finding of a linear, non-axisymmetric, global instability in gas discs around stars, which may be relevant to other astrophysical discs. It takes the form of an

astro-ph.EP20253 cited

On the formation of multiple dust-trapping rings in the inner Solar system

E. Lega, A. Morbidelli, F. Masset +1

Isotopic properties of meteorites provide evidence that multiple dust trap or pressure bumps had to form and persist in the inner Solar System on a timescale of millions of years.…

astro-ph.EP20253 cited

Dust-void evolution driven by turbulent dust flux can induce runaway migration of Earth-mass planets

R. O. Chametla, O. Chrenko, F. S. Masset +2

Torques from asymmetric dust structures (so-called dust-void and filamentary structures) formed around low-mass planets embedded in a non turbulent dust-gas disk can exceed the tor…

astro-ph.EP2024

A close pair of orbiters embedded in a gaseous disk: the repulsive effect

F. J. Sanchez-Salcedo, F. S. Masset, S. Cornejo

We develop a theoretical framework and use two-dimensional hydrodynamical simulations to study the repulsive effect between two close orbiters embedded in an accretion disk. We con…