activity
20152026
most citedPhantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics

431 citations · 1.2k across the 44 of their papers we have counts for

collaborators
Showing 2019Show all

6 papers · 1 filter

astro-ph.EP2019★ 29 cited

Flyby-induced misalignments in planet-hosting discs

Rebecca Nealon, Nicolás Cuello, Richard Alexander

We now have several observational examples of misaligned broken protoplanetary discs, where the disc inner regions are strongly misaligned with respect to the outer disc. Current m…

astro-ph.EP2019★ 79 cited

Flybys in protoplanetary discs: II. Observational signatures

Nicolás Cuello, Fabien Louvet, Daniel Mentiplay +14

Tidal encounters in star clusters perturb discs around young protostars. In Cuello et al. (2019a, Paper I) we detailed the dynamical signatures of a stellar flyby in both gas and d…

astro-ph.HE2019★ 17 cited

Gravitational wave emission from unstable accretion discs in tidal disruption events

M. Toscani, G. Lodato, R. Nealon

Gravitational waves can be emitted by accretion discs if they undergo instabilities that generate a time varying mass quadrupole. In this work we investigate the gravitational sign…

astro-ph.GA2019★ 10 cited

Supermassive Black Hole Demographics: Evading

Andrew King, Rebecca Nealon

We consider black hole - galaxy coevolution using simple analytic arguments. We focus on the fact that several supermassive black holes are known with masses significantly larger t…

astro-ph.HE2019★ 48 cited

Generalised warped disk equations

Rebecca G. Martin, Stephen H. Lubow, J. E. Pringle +6

The manner in which warps in accretion disks evolve depends on the magnitude of the viscosity. For small viscosity the warp evolves in a wave-like manner; for large visc…

astro-ph.EP2019★ 61 cited

Scattered light shadows in warped protoplanetary discs

Rebecca Nealon, Christophe Pinte, Richard Alexander +2

Three-dimensional hydrodynamic numerical simulations have demonstrated that the structure of a protoplanetary disc may be strongly affected by a planet orbiting in a plane that is…