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20212024
most citedDisks in close binary stars: γ-Cephei revisited

12 citations · 31 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2024★ 1 cited

Hydrodynamical simulations with strong indirect terms in Fargo-like codes: Numerical aspects of non-inertial frame and artificial viscosity

Lucas M. Jordan, Thomas Rometsch

Context. Binary star systems allow us to study the planet formation process under extreme conditions. In the early stages, these systems contain a circumbinary disk and a disk arou…

astro-ph.HE2024★ 11 cited

Two-dimensional simulations of disks in close binaries: Simulating outburst cycles in cataclysmic variables

Lucas M. Jordan, Dennis Wehner, Rolf Kuiper

Previous simulations of cataclysmic variables studied either the quiescence, or the outburst state in multiple dimensions or they simulated complete outburst cycles in one dimensio…

astro-ph.EP2024

FargoCPT: A 2D Multi-Physics Code for Simulating the Interaction of Disks with Stars, Planets and Particles

Thomas Rometsch, Lucas M. Jordan, Tobias W. Moldenhauer +6

Context: Planet-disk interactions play a crucial role in the understanding of planet formation and disk evolution. There are multiple numerical tools available to simulate these in…

astro-ph.IM2023★ 2 cited

Measuring the Numerical Viscosity in Simulations of Protoplanetary Disks in Cartesian Grids -- The Viscously Spreading Ring Revisited

Jibin Joseph, Alexandros Ziampras, Lucas Jordan +2

Hydrodynamical simulations solve the governing equations on a discrete grid of space and time. This discretization causes numerical diffusion similar to a physical viscous diffusio…

astro-ph.GA2023★ 5 cited

The rotational disruption of porous dust aggregates from ab-initio kinematic calculations

Stefan Reissl, Philipp Nguyen, Lucas M. Jordan +1

Context: The sizes of dust in the interstellar medium follows a distribution where most of the dust mass is in smaller grains. However, the re-distribution from larger grains towar…

astro-ph.EP2021★ 12 cited

Disks in close binary stars: γ-Cephei revisited

Lucas M. Jordan, Wilhelm Kley, Giovanni Picogna +1

Close binaries ( au) are known to harbor planets, yet planet formation is unlikely to succeed in such systems. Studying the dynamics of disks in close binaries can he…