activity
20182021
most citedA new class of Super-Earths formed from high-temperature condensates: HD219134 b, 55 Cnc e, WASP-47 e

97 citations · 264 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.EP202143 cited

Bayesian constraints on the origin and geology of exo-planetary material using a population of externally polluted white dwarfs

John H. D. Harrison, Amy Bonsor, Mihkel Kama +3

White dwarfs that have accreted planetary bodies are a powerful probe of the bulk composition of exoplanetary material. In this paper, we present a Bayesian model to explain the ab…

astro-ph.EP202119 cited

Evidence for post-nebula volatilisation in an exo-planetary body

John H. D. Harrison, Oliver Shorttle, Amy Bonsor

The loss and gain of volatile elements during planet formation is key for setting their subsequent climate, geodynamics, and habitability. Two broad regimes of volatile element tra…

astro-ph.EP202040 cited

Exocomets from a Solar System Perspective

Paul A. Strøm, Dennis Bodewits, Matthew M. Knight +24

Exocomets are small bodies releasing gas and dust which orbit stars other than the Sun. Their existence was first inferred from the detection of variable absorption features in ste…

astro-ph.EP202065 cited

Are exoplanetesimals differentiated?

Amy Bonsor, Philip J. Carter, Mark Hollands +3

Metals observed in the atmospheres of white dwarfs suggest that many have recently accreted planetary bodies. In some cases, the compositions observed suggest the accretion of mate…

astro-ph.EP201897 cited

A new class of Super-Earths formed from high-temperature condensates: HD219134 b, 55 Cnc e, WASP-47 e

Caroline Dorn, John H. D. Harrison, Amy Bonsor +1

We hypothesise that differences in the temperatures at which the rocky material condensed out of the nebula gas can lead to differences in the composition of key rocky species (e.g…

astro-ph.EP2018

Polluted White Dwarfs: Constraints on the Origin and Geology of Exoplanetary Material

John H. D. Harrison, Amy Bonsor, Nikku Madhusudhan

White dwarfs that have accreted rocky planetary bodies provide unique insights regarding the bulk composition of exoplanetary material. The analysis presented here uses observed wh…