activity
20142016
most citedHydrogen delivery onto white dwarfs from remnant exo-Oort cloud comets

89 citations · 266 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP201647 cited

The unseen planets of double belt debris disk systems

Andrew Shannon, Amy Bonsor, Quentin Kral +1

The gap between two component debris disks is often taken to be carved by intervening planets scattering away the remnant planetesimals. We employ N-body simulations to determine h…

astro-ph.EP201525 cited

Capture and evolution of dust in planetary mean-motion resonances: a fast, semi-analytic method for generating resonantly trapped disk images

Andrew Shannon, Alexander J Mustill, Mark Wyatt

Dust grains migrating under Poynting-Robertson drag may be trapped in mean-motion resonances with planets. Such resonantly trapped grains are observed in the solar system. In extra…

astro-ph.EP201438 cited

Exo-zodi modelling for the Large Binocular Telescope Interferometer

Grant M. Kennedy, Mark C. Wyatt, Vanessa Bailey +18

Habitable zone dust levels are a key unknown that must be understood to ensure the success of future space missions to image Earth analogues around nearby stars. Current detection…

astro-ph.EP201446 cited

Eight billion asteroids in the Oort cloud

Andrew Shannon, Alan P. Jackson, Dimitri Veras +1

The Oort cloud is usually thought of as a collection of icy comets inhabiting the outer reaches of the Solar system, but this picture is incomplete. We use simulations of the forma…

astro-ph.SR201489 cited

Hydrogen delivery onto white dwarfs from remnant exo-Oort cloud comets

Dimitri Veras, Andrew Shannon, Boris T. Gaensicke

The origin of trace hydrogen in white dwarfs (WDs) with He-dominated atmospheres is a long-standing problem, one that cannot satisfactorily be explained by the historically-favoure…

astro-ph.EP201421 cited

Dancing with the Stars: Formation of the Fomalhaut triple system and its effect on the debris disks

Andrew Shannon, Cathie Clarke, Mark Wyatt

Fomalhaut is a triple system, with all components widely separated (~1E5 au). Such widely separated binaries are thought to form during cluster dissolution, but that process is unl…