activity
20242026
most citedDiscovery of an icy and nitrogen-rich extrasolar planetesimal

4 citations · 13 across the 15 of their papers we have counts for

collaborators

17 papers

astro-ph.EP2026

Where planetary solids survive sublimation around young and hot white dwarfs

Dimitri Veras, Keiji Ohtsuki, Rafael Martinez-Brunner +2

All observed planetary systems orbiting single white dwarfs have lived through the hot stellar transition from an asymptotic giant branch star. In this post-nebular transition peri…

astro-ph.EP2026

White dwarf planets in star clusters: gravitational scattering versus mass-loss effects

Richard J. Parker, Dimitri Veras

White dwarfs are unique laboratories for understanding the formation, evolution and survivability of planetary systems. Post-main sequence mass-loss will change planetary orbital p…

astro-ph.EP2026

Size limits on tidal debris around white dwarfs: the km-size barrier

Jordan K. Steckloff, Dimitri Veras, Kathryn Volk

Compact disks of planetary debris orbiting white dwarfs provide a crucial window into our understanding of evolved planetary systems. The formation of these disks has been widely m…

astro-ph.IM2026

DebrisWatch II: Digging deeper for geosynchronous debris

James A. Blake, Benjamin F. Cooke, Cristina Paragini +27

The geosynchronous (GSO) debris environment is continually evolving. Regular monitoring of the region is consequently of great importance, though the trade-off between coverage and…

astro-ph.EP2026

Producing planetary debris exterior to white dwarf Roche radii through sublimative rotational fission

Dimitri Veras, Jordan K. Steckloff, Kathryn Volk

The majority of white dwarfs that host periodic transiting planetary debris do so at distances that exceed the rubble-pile Roche limit, in disagreement with canonical formation mod…

astro-ph.EP2026

The evolution of exocomets and their source populations

Alexander J. Mustill, Tim Pearce, Michele Bannister +12

We review the current state of knowledge of the long-term evolution of the small bodies that give rise to comets and exocomets, as well as their reservoirs. The active cometary pha…

astro-ph.EP2026

Exocometary physics: material release and tails

Théo Vrignaud, Dennis Bodewits, Jake Hanlon +5

Despite decades of observations, the physical processes governing mass loss from small bodies beyond our Solar System remain poorly constrained. These exocomets are often treated a…

astro-ph.IM2025

The Future of Evolved Planetary Systems

Roberto Raddi, Anna F. Pala, Alberto Rebassa-Mansergas +19

Understanding the formation, evolution, and chemical diversity of exoplanets are now central areas of astrophysics research. White dwarfs provide a uniquely sensitive laboratory fo…

astro-ph.EP2025

The Origins & Reservoirs of Exocomets

Michele Bannister, Susanne Pfalzner, Tim Pearce +11

Small bodies exist in distinct populations within their planetary systems. These reservoir populations hold a range of compositions, which to first order are dependent on formation…

astro-ph.EP2025★ 4 cited

Discovery of an icy and nitrogen-rich extrasolar planetesimal

Snehalata Sahu, Boris T. Gänsicke, Jamie T. Williams +7

White dwarfs accreting planetary debris provide detailed insight into the bulk composition of rocky exo-planetesimals. However, only one Kuiper-Belt analogue has been identified in…

astro-ph.SR2025★ 1 cited

Transiting Planetary Debris near the Roche Limit of a White Dwarf on a 4.97hr Orbit -- and its Vanishing

Joseph A. Guidry, Zachary P. Vanderbosch, J. J. Hermes +9

We present the discovery of deep, irregular, periodic transits towards the white dwarf ZTFJ19444557 using follow-up time-series photometry and spectroscopy from Palomar, Kec…

astro-ph.EP2025

Bounding destruction timescales of minor planets orbiting white dwarfs with the sesquinary catastrophe

Dimitri Veras, Matija Ćuk

Dynamical activity attributed to the destruction of minor planets orbiting white dwarfs has now been photometrically monitored in individual systems for up to one decade, long enou…

astro-ph.EP2025

Resupplying planetary debris to old white dwarfs with supernova blast waves

Dimitri Veras

One challenge with explaining how high levels of planetary debris can enrich, or "pollute", old (3 Gyr) and very old (10 Gyr) white dwarfs is that debris reservoirs dep…

astro-ph.SR2025★ 4 cited

Characterizing planetary material accreted by cool helium atmosphere white dwarfs using an exponentially decaying disc model

Mairi W. O'Brien, Pier-Emmanuel Tremblay, Beth L. Klein +5

We present Keck High Resolution Echelle Spectrometer (HIRES) observations and model atmosphere analysis for two nearby, cool, helium-dominated atmosphere white dwarfs that have bee…

astro-ph.SR2025

The dearth of high-mass hydrogen-atmosphere metal-polluted white dwarfs within 40 pc

Tim Cunningham, Pier-Emmanuel Tremblay, Mairi O'Brien +7

We present a population synthesis model which addresses the different mass distributions of the metal-polluted and non-metal-polluted hydrogen-atmosphere white dwarfs identified in…

astro-ph.EP2024

Simultaneous emission from dust and gas in the planetary debris orbiting a white dwarf

Laura K. Rogers, Christopher J. Manser, Amy Bonsor +11

There is increasing evidence for the presence and variability of circumstellar dust and gas around white dwarfs that are polluted with exoplanetary material, although the origin of…

astro-ph.EP2024★ 4 cited

The evolution and delivery of rocky extra-solar materials to white dwarfs

Dimitri Veras, Alexander J. Mustill, Amy Bonsor

Understanding stellar evolution and its effect on planetary systems is crucial for correctly interpreting the chemical constraints of exo-planetary material that can be given to us…