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20182026
most citedDebris Disks: Structure, Composition, and Variability

324 citations · 688 across the 11 of their papers we have counts for

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6 papers · 1 filter

astro-ph.EP2026

Binary tidal evolution as a sculptor of circumbinary planet architectures

Mario Sucerquia, Nicolás Cuello, Gaspard Duchêne

Circumbinary planets (CBPs) are expected to form in circumbinary discs and migrate towards the disc inner cavity, often near the binary stability boundary. Yet the observed populat…

astro-ph.EP2026

The dust in Sauron's eye - Observational and experimental results on the debris disk around HR 4796

M. Bonduelle, J. Milli, O. Poch +14

The optical properties (scattering phase function SPF; degree of linear polarization DoLP; reflectance) of the dust particles orbiting in debris disks can be retrieved through scat…

astro-ph.EP2025★ 6 cited

The role of absorption and scattering in shaping ice bands. Spatially-resolved spectroscopy of protoplanetary disks

Laurine Martinien, Gaspard Duchêne, François Ménard +2

The James Webb Space Telescope now enables the spectral study of ices with unprecedented sensitivity and angular resolution. Water ice plays a crucial role in the growth of grains…

astro-ph.EP2024★ 14 cited

Running with the Bulls: The frequency of star-disc encounters in the Taurus star forming region

Andrew J. Winter, Myriam Benisty, Linling Shuai +5

Stars and planets form in regions of enhanced stellar density, subjecting protoplanetary discs to gravitational perturbations from neighbouring stars. Observations in the Taurus st…

astro-ph.EP2024★ 13 cited

Orbital dynamics in the GG Tau A system: investigating its enigmatic disc

Claudia Toci, Simone Ceppi, Nicolás Cuello +6

GG Tau is one of the most studied multiple young stellar systems: GG Tau A is a hierarchical triple surrounded by a massive disc and its companion, GG Tau B, is also a binary. Desp…

astro-ph.EP2018★ 324 cited

Debris Disks: Structure, Composition, and Variability

A. Meredith Hughes, Gaspard Duchene, Brenda Matthews

Debris disks are tenuous, dust-dominated disks commonly observed around stars over a wide range of ages. Those around main sequence stars are analogous to the Solar System's Kuiper…